This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr
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 22.0978 2461093.5978 11.46 23:16:48.90 +54:33:26.6
109.40656 -5.81049 galactic Cas 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 1996792319540411776 | 23:16:48.96 +54:33:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 48.90 +54 33 26.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996792319540411776,2461093.5978,11.46,0.05,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 1996792319540411776 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:48.90 +54:33:26.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.41 23:24:26.64 +50:09:59.2
108.97096 -10.33232 galactic And Second-epoch detections are separated by 6.8" 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 1943149243164039936 | 23:24:26.20 +50:09:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 24 26.64 +50 09 59.2 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943149243164039936,2461093.5978,11.41,0.05,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 1943149243164039936 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:24:26.64 +50:09:59.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.27 23:15:58.43 +52:22:28.7
108.49504 -7.80070 galactic And Second-epoch detections are separated by 7.3" 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 1992258448985850112 | 23:15:59.13 +52:22:32.5 (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!
TCP 2026 02 22.0978* 23 15 58.43 +52 22 28.7 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992258448985850112,2461093.5978,11.27,0.05,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 1992258448985850112 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:15:58.43 +52:22:28.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 26 12.57 +54 32 12.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232612.99+543157.1,2461093.5978,11.18,0.05,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
ZTF J232612.99+543157.1 20260222.0978 11.18CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:12.57 +54:32:12.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.13 23:33:18.60 +49:25:54.1
110.11256 -11.48553 galactic And 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 | Gaia DR3 1942158583187895040 | 23:33:19.08 +49:25:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 33 18.60 +49 25 54.1 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942158583187895040,2461093.5978,11.13,0.05,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 1942158583187895040 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:18.60 +49:25:54.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.08 23:28:56.01 +57:57:15.8
112.14253 -3.17862 galactic Cas Second-epoch detections are separated by 3.5" 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 | ATO J352.2476+57.9548 | 23:28:55.42 +57:57:21.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 28 56.01 +57 57 15.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.2476+57.9548,2461093.5978,11.08,0.05,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
ATO J352.2476+57.9548 20260222.0978 11.08CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:28:56.01 +57:57:15.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.93 23:24:03.02 +57:21:01.3
111.32789 -3.53933 galactic Cas Second-epoch detections are separated by 3.1" 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 2009363757534620928 | 23:24:02.41 +57:20:50.1 (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!
TCP 2026 02 22.0978* 23 24 03.02 +57 21 01.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009363757534620928,2461093.5978,10.93,0.05,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 2009363757534620928 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:24:03.02 +57:21:01.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.94 23:28:22.33 +49:35:07.3
109.38513 -11.08899 galactic And Second-epoch detections are separated by 1.4" 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 | ATO J352.0780+49.5772 | 23:28:21.91 +49:35:02.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1952CoRut..32....1H BD+48 4060
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 28 22.33 +49 35 07.3 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.0780+49.5772,2461093.5978,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.0780+49.5772 20260222.0978 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:28:22.33 +49:35:07.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 25 18.02 +56 06 27.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997036033166700544,2461093.5978,10.77,0.05,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 1997036033166700544 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:18.02 +56:06:27.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.74 23:21:43.73 +50:16:58.3
108.59622 -10.07517 galactic And Second-epoch detections are separated by 4.5" 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 1991185634871214208 | 23:21:43.20 +50:16:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1932MeUpp..55....1S BD+49 4097
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 21 43.73 +50 16 58.3 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991185634871214208,2461093.5978,10.74,0.05,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 1991185634871214208 20260222.0978 10.74CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:43.73 +50:16:58.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.35 23:26:51.31 +50:08:05.1
109.33090 -10.49002 galactic And 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 1943186420399844608 | 23:26:50.67 +50:07:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1952CoRut..32....1H BD+49 4121
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 26 51.31 +50 08 05.1 10.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943186420399844608,2461093.5978,10.35,0.05,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 1943186420399844608 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:51.31 +50:08:05.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 9.35 23:06:21.65 +57:32:45.6
109.17939 -2.49285 galactic Cas 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 | ATO J346.5676+57.5379 | 23:06:20.44 +57:32:46.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=VARIABLE SpType: K5 1947AnDea...5....1L DO 42495
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 21.65 +57 32 45.6 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.5676+57.5379,2461093.5978,9.35,0.05,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
ATO J346.5676+57.5379 20260222.0978 9.35CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:21.65 +57:32:45.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 16.74 +56 18 24.7 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009040707277065344,2461093.5978,9.70,0.05,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 2009040707277065344 20260222.0978 9.70CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:16.74 +56:18:24.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 9.92 23:08:10.63 +58:15:54.3
109.68299 -1.92536 galactic Cas Second-epoch detections are separated by 7.2" 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 2010216016487968384 | 23:08:09.36 +58:15:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3 1958ApJ...128..510N BD+57 2698
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 10.63 +58 15 54.3 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010216016487968384,2461093.5978,9.92,0.05,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 2010216016487968384 20260222.0978 9.92CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:10.63 +58:15:54.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.02 23:23:34.51 +49:16:56.8
108.53301 -11.11718 galactic And 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 1942845709234434688 | 23:23:35.25 +49:17:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+48 4024
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 23 34.51 +49 16 56.8 10.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942845709234434688,2461093.5978,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1942845709234434688 20260222.0978 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:34.51 +49:16:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.18 23:14:29.46 +51:30:48.1
107.96141 -8.51833 galactic And Second-epoch detections are separated by 7.3" 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 1991958763344445056 | 23:14:30.22 +51:30:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 29.46 +51 30 48.1 10.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991958763344445056,2461093.5978,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991958763344445056 20260222.0978 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:29.46 +51:30:48.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.20 23:14:32.26 +53:17:07.5
108.62723 -6.87367 galactic Cas Second-epoch detections are separated by 4.9" 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 | ATO J348.6483+53.2794 | 23:14:34.07 +53:17:04.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1927AnHar.100...33C HD 236074
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 32.26 +53 17 07.5 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.6483+53.2794,2461093.5978,10.20,0.05,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
ATO J348.6483+53.2794 20260222.0978 10.20CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:32.26 +53:17:07.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.21 23:31:50.68 +58:46:18.2
112.75863 -2.51900 galactic Cas Second-epoch detections are separated by 1.3" 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 2011178020439517056 | 23:31:52.12 +58:46:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 240322
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 31 50.68 +58 46 18.2 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2011178020439517056,2461093.5978,10.21,0.05,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 2011178020439517056 20260222.0978 10.21CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:31:50.68 +58:46:18.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.25 23:18:07.49 +54:06:43.0
109.42612 -6.29473 galactic Cas 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 1995968750970990336 | 23:18:08.80 +54:06:47.6 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A2 1927AnHar.100...33C HD 236093
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 07.49 +54 06 43.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995968750970990336,2461093.5978,10.25,0.05,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
Gaia DR3 1995968750970990336 20260222.0978 10.25CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:07.49 +54:06:43.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 51.50 +51 00 45.1 10.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991144849862320384,2461093.5978,10.26,0.05,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 1991144849862320384 20260222.0978 10.26CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:51.50 +51:00:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.16 23:36:09.46 +58:47:01.4
113.29672 -2.67260 galactic Cas Second-epoch detections are separated by 8.0" 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 | ATO J354.0516+58.7895 | 23:36:10.17 +58:46:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1928AnHar.100...49C HD 240338
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 36 09.46 +58 47 01.4 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.0516+58.7895,2461093.5978,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.0516+58.7895 20260222.0978 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:36:09.46 +58:47:01.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.43 23:22:44.87 +48:59:09.0
108.30020 -11.34988 galactic And Second-epoch detections are separated by 1.9" 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 1942837600336286464 | 23:22:45.41 +48:59:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3V 1928MeUpp..37....1S BD+48 4019
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 22 44.87 +48 59 09.0 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942837600336286464,2461093.5978,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1942837600336286464 20260222.0978 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:44.87 +48:59:09.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 33.86 +54 23 59.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996022317804843136,2461093.5978,10.29,0.05,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 1996022317804843136 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:33.86 +54:23:59.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.37 23:23:13.06 +57:09:34.0
111.15776 -3.68180 galactic Cas Second-epoch detections are separated by 3.5" 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 | ATO J350.8019+57.1544 | 23:23:14.26 +57:09:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1928AnHar.100...49C HD 240278
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 23 13.06 +57 09 34.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.8019+57.1544,2461093.5978,10.37,0.05,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
ATO J350.8019+57.1544 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:13.06 +57:09:34.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 10 55.86 +53 27 56.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995596531929802880,2461093.5978,10.35,0.05,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 1995596531929802880 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:10:55.86 +53:27:56.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.41 23:18:45.44 +51:22:46.1
108.53927 -8.88373 galactic And Second-epoch detections are separated by 7.7" 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 | Large-amplitude variable Gaia DR2 1992281813598481280 | 23:18:46.03 +51:22:51.8 (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: A0 1927AnHar.100...33C HD 236097
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 45.44 +51 22 46.1 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1992281813598481280,2461093.5978,10.41,0.05,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
Large-amplitude variable Gaia DR2 1992281813598481280 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:45.44 +51:22:46.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 15 50.31 +57 32 36.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FN Cas,2461093.5978,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FN Cas 20260222.0978 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:15:50.31 +57:32:36.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.41 23:25:05.09 +58:25:07.5
111.81074 -2.57607 galactic Cas 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 2009658667167540224 | 23:25:06.33 +58:25:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1928AnHar.100...49C HD 240296
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 25 05.09 +58 25 07.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009658667167540224,2461093.5978,10.41,0.05,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 2009658667167540224 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:05.09 +58:25:07.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.39 23:15:50.84 +52:57:36.9
108.69170 -7.24816 galactic And Second-epoch detections are separated by 3.6" 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 | ATO J348.9601+52.9506 | 23:15:51.87 +52:57:37.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1927AnHar.100...33C HD 236076
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 15 50.84 +52 57 36.9 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.9601+52.9506,2461093.5978,10.39,0.05,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
ATO J348.9601+52.9506 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:15:50.84 +52:57:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.44 23:06:19.18 +57:19:32.8
109.08735 -2.69304 galactic Cas Second-epoch detections are separated by 8.9" 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 2009906607042342784 | 23:06:18.65 +57:19:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1928AnHar.100...49C HD 240187
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 19.18 +57 19 32.8 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009906607042342784,2461093.5978,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009906607042342784 20260222.0978 10.44CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:19.18 +57:19:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 04 39.84 +58 34 38.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3478265,2461093.5978,10.45,0.05,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 3478265 20260222.0978 10.45CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:04:39.84 +58:34:38.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.34 23:30:07.22 +49:12:19.0
109.53662 -11.53988 galactic And Second-epoch detections are separated by 8.0" 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 | ATO J352.5147+49.2036 | 23:30:07.68 +49:12:25.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K 1952CoRut..32....1H BD+48 4068
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 30 07.22 +49 12 19.0 10.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.5147+49.2036,2461093.5978,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.5147+49.2036 20260222.0978 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:30:07.22 +49:12:19.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.45 23:12:38.78 +53:54:03.1
108.59469 -6.19804 galactic Cas Second-epoch detections are separated by 2.2" 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 | ATO J348.1698+53.8902 | 23:12:39.79 +53:54:04.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 38.78 +53 54 03.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1698+53.8902,2461093.5978,10.45,0.05,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
ATO J348.1698+53.8902 20260222.0978 10.45CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:38.78 +53:54:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.49 23:16:03.91 +52:59:24.8
108.73347 -7.23214 galactic And Second-epoch detections are separated by 3.6" 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 | ATO J349.0161+52.9805 | 23:16:05.00 +52:59:20.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B AG+52 1739
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 03.91 +52 59 24.8 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.0161+52.9805,2461093.5978,10.49,0.05,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
ATO J349.0161+52.9805 20260222.0978 10.49CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:03.91 +52:59:24.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.49 23:18:09.27 +58:40:45.9
111.04873 -2.02343 galactic Cas Second-epoch detections are separated by 0.8" 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 | ATO J349.5347+58.6857 | 23:18:10.43 +58:40:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1928AnHar.100...49C HD 240251
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 09.27 +58 40 45.9 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.5347+58.6857,2461093.5978,10.49,0.05,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
ATO J349.5347+58.6857 20260222.0978 10.49CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:09.27 +58:40:45.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.51 23:19:41.13 +53:03:08.3
109.26863 -7.36806 galactic And Second-epoch detections are separated by 7.5" 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 1992665268279395328 | 23:19:41.83 +53:03:10.5 (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!
TCP 2026 02 22.0978* 23 19 41.13 +53 03 08.3 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992665268279395328,2461093.5978,10.51,0.05,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 1992665268279395328 20260222.0978 10.51CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:41.13 +53:03:08.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.54 23:11:44.96 +51:11:15.3
107.43661 -8.66014 galactic And Second-epoch detections are separated by 5.7" 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 1991950139051058688 | 23:11:45.91 +51:11:22.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+50 3979
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 11 44.96 +51 11 15.3 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991950139051058688,2461093.5978,10.54,0.05,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 1991950139051058688 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:11:44.96 +51:11:15.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.55 23:23:32.54 +57:39:03.3
111.36360 -3.23320 galactic Cas Second-epoch detections are separated by 7.2" 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 2009432854968312576 | 23:23:33.78 +57:39:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 23 32.54 +57 39 03.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009432854968312576,2461093.5978,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009432854968312576 20260222.0978 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:32.54 +57:39:03.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.63 23:21:09.78 +49:01:55.5
108.06779 -11.21671 galactic And Second-epoch detections are separated by 3.1" 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 | ATO J350.2798+49.0296 | 23:21:10.20 +49:01:60.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+48 4007
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 21 09.78 +49 01 55.5 10.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.2798+49.0296,2461093.5978,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.2798+49.0296 20260222.0978 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:09.78 +49:01:55.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.60 23:08:32.28 +53:33:12.4
107.89634 -6.28746 galactic Cas Second-epoch detections are separated by 1.4" 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 1995516744313401472 | 23:08:31.67 +53:33:07.1 (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!
TCP 2026 02 22.0978* 23 08 32.28 +53 33 12.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995516744313401472,2461093.5978,10.60,0.05,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 1995516744313401472 20260222.0978 10.60CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:32.28 +53:33:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.65 23:21:27.78 +58:22:08.2
111.34641 -2.46437 galactic Cas Second-epoch detections are separated by 3.2" 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 2009690896598204160 | 23:21:29.92 +58:22:07.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1928AnHar.100...49C HD 240271
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 21 27.78 +58 22 08.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009690896598204160,2461093.5978,10.65,0.05,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 2009690896598204160 20260222.0978 10.65CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:27.78 +58:22:08.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 20 24.77 +55 31 27.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996904534146902144,2461093.5978,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996904534146902144 20260222.0978 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:24.77 +55:31:27.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.55 23:06:36.13 +57:42:22.9
109.27232 -2.35817 galactic Cas 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 | ATO J346.6429+57.6955 | 23:06:37.21 +57:42:19.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8III 1954UppAn...4a...1M BD+56 2948
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 36.13 +57 42 22.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.6429+57.6955,2461093.5978,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.6429+57.6955 20260222.0978 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:36.13 +57:42:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.72 23:29:47.18 +58:29:35.6
112.41787 -2.70182 galactic Cas 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 | ATO J352.4620+58.4876 | 23:29:48.44 +58:29:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1955IzKry..14....3B [B55b] 3122
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 29 47.18 +58 29 35.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.4620+58.4876,2461093.5978,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.4620+58.4876 20260222.0978 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:29:47.18 +58:29:35.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.72 23:23:31.53 +49:00:05.7
108.42799 -11.37860 galactic And Second-epoch detections are separated by 4.2" 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 1942826880097953024 | 23:23:33.12 +49:00:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1958PMcCO..13b....V AG+48 2056
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 23 31.53 +49 00 05.7 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942826880097953024,2461093.5978,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1942826880097953024 20260222.0978 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:31.53 +49:00:05.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 00.21 +50 50 51.8 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 03648-01384,2461093.5978,10.75,0.05,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
GSC 03648-01384 20260222.0978 10.75CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:00.21 +50:50:51.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 41.17 +58 18 06.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2308401+581809,2461093.5978,10.69,0.05,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
NSVS J2308401+581809 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:41.17 +58:18:06.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.76 23:12:25.34 +53:51:03.9
108.54515 -6.23183 galactic Cas 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 1995640821631104896 | 23:12:26.42 +53:51:12.0 (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!
TCP 2026 02 22.0978* 23 12 25.34 +53 51 03.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995640821631104896,2461093.5978,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995640821631104896 20260222.0978 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:25.34 +53:51:03.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.71 23:20:44.78 +57:52:27.7
111.08800 -2.89672 galactic Cas Second-epoch detections are separated by 1.9" 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 | ATO J350.1938+57.8637 | 23:20:45.50 +57:52:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1928AnHar.100...49C HD 240265
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 20 44.78 +57 52 27.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.1938+57.8637,2461093.5978,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.1938+57.8637 20260222.0978 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:44.78 +57:52:27.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 44 42.32 +48 36 30.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004442.78+483626.6,2461093.5978,11.08,0.05,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
ASASSN-V J004442.78+483626.6 20260222.0978 11.08CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:42.32 +48:36:30.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.71 23:06:53.84 +56:42:52.0
108.91878 -3.28597 galactic Cas Second-epoch detections are separated by 1.8" 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 | ATO J346.7401+56.7163 | 23:06:54.68 +56:42:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B3 1928AnHar.100...49C HD 240190
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 53.84 +56 42 52.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.7401+56.7163,2461093.5978,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.7401+56.7163 20260222.0978 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:53.84 +56:42:52.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 26 31.38 +49 29 39.6 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 14561,2461093.5978,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 14561 20260222.0978 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:31.38 +49:29:39.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.67 23:12:22.31 +52:05:19.2
107.87103 -7.86236 galactic And Second-epoch detections are separated by 6.0" 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 | ATO J348.1015+52.0996 | 23:12:22.70 +52:05:32.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1984AJ.....89..702L BD+51 3557
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 22.31 +52 05 19.2 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1015+52.0996,2461093.5978,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.1015+52.0996 20260222.0978 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:22.31 +52:05:19.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 00.28 +54 37 16.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996474629402785152,2461093.5978,10.75,0.05,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
Gaia DR3 1996474629402785152 20260222.0978 10.75CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:00.28 +54:37:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 14.19 +49 05 42.7 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1990736656169640576,2461093.5978,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1990736656169640576 20260222.0978 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:14.19 +49:05:42.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.80 23:11:30.90 +50:56:33.5
107.30801 -8.87274 galactic And Second-epoch detections are separated by 2.3" 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 1991838504261886848 | 23:11:31.43 +50:56:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0III 1932MeUpp..55....1S BD+50 3977
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 11 30.90 +50 56 33.5 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991838504261886848,2461093.5978,10.80,0.05,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
Gaia DR3 1991838504261886848 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:11:30.90 +50:56:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 07 09.31 +58 33 17.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SW Cas,2461093.5978,10.81,0.05,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
SW Cas 20260222.0978 10.81CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:09.31 +58:33:17.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 43.94 +55 52 27.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008828428510569472,2461093.5978,10.81,0.05,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
Gaia DR3 2008828428510569472 20260222.0978 10.81CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:43.94 +55:52:27.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 15 16.53 +55 01 21.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996861932371603584,2461093.5978,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996861932371603584 20260222.0978 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:15:16.53 +55:01:21.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 37 40.16 +58 50 41.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0850 Cas,2461093.5978,10.91,0.05,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
V0850 Cas 20260222.0978 10.91CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:40.16 +58:50:41.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.91 23:20:10.60 +58:47:09.3
111.33197 -2.01518 galactic Cas Second-epoch detections are separated by 0.9" 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 2010467839007425792 | 23:20:11.66 +58:47:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1935BSD...C01....0S BSD 19- 86
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 20 10.60 +58 47 09.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010467839007425792,2461093.5978,10.91,0.05,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 2010467839007425792 20260222.0978 10.91CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:10.60 +58:47:09.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.95 23:19:32.11 +49:23:44.2
107.94416 -10.78302 galactic And Second-epoch detections are separated by 8.4" 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 1942721876739305472 | 23:19:32.73 +49:23:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+48 3998
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 19 32.11 +49 23 44.2 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942721876739305472,2461093.5978,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1942721876739305472 20260222.0978 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:32.11 +49:23:44.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.88 23:10:52.61 +50:48:05.3
107.15928 -8.96480 galactic And Second-epoch detections are separated by 0.5" 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 | ATO J347.7054+50.7993 | 23:10:52.10 +50:47:59.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 10 52.61 +50 48 05.3 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.7054+50.7993,2461093.5978,10.88,0.05,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
ATO J347.7054+50.7993 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:10:52.61 +50:48:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.94 23:12:29.99 +50:52:36.3
107.42819 -8.99251 galactic And Second-epoch detections are separated by 2.0" 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 | ATO J348.1162+50.8773 | 23:12:31.00 +50:52:42.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 1932MeUpp..55....1S BD+50 3983
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 29.99 +50 52 36.3 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1162+50.8773,2461093.5978,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.1162+50.8773 20260222.0978 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:29.99 +50:52:36.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.90 23:03:33.01 +57:59:54.1
109.01620 -1.92853 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J345.8723+57.9997 | 23:03:34.14 +57:59:48.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 03 33.01 +57 59 54.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J345.8723+57.9997,2461093.5978,10.90,0.05,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
ATO J345.8723+57.9997 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:03:33.01 +57:59:54.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.93 23:08:26.67 +55:49:47.7
108.77110 -4.18419 galactic Cas Second-epoch detections are separated by 3.4" 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 | ATO J347.0951+55.8319 | 23:08:27.40 +55:49:45.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 240196
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 26.67 +55 49 47.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.0951+55.8319,2461093.5978,10.93,0.05,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
ATO J347.0951+55.8319 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:26.67 +55:49:47.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 19 53.05 +56 57 33.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009331218861877760,2461093.5978,10.98,0.05,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
Gaia DR3 2009331218861877760 20260222.0978 10.98CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:53.05 +56:57:33.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.02 23:34:48.15 +58:51:33.3
113.15060 -2.54946 galactic Cas Second-epoch detections are separated by 0.4" 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 2011087551242246016 | 23:34:49.45 +58:51:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 1935BSD...C01....0S BSD 19- 221
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 34 48.15 +58 51 33.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2011087551242246016,2461093.5978,11.02,0.05,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
Gaia DR3 2011087551242246016 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:34:48.15 +58:51:33.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.96 23:21:30.88 +57:53:52.7
111.19216 -2.90947 galactic Cas Second-epoch detections are separated by 0.3" 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 2009617985238380160 | 23:21:31.62 +57:53:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 21 30.88 +57 53 52.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009617985238380160,2461093.5978,10.96,0.05,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
Gaia DR3 2009617985238380160 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:30.88 +57:53:52.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 22 03.16 +58 13 01.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009674025970572928,2461093.5978,10.88,0.05,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
Gaia DR3 2009674025970572928 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:03.16 +58:13:01.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.94 23:11:38.84 +58:43:39.5
110.27884 -1.67086 galactic Cas Second-epoch detections are separated by 0.6" 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 2010607369606567040 | 23:11:40.18 +58:43:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1928AnHar.100...49C HD 240219
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 11 38.84 +58 43 39.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010607369606567040,2461093.5978,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2010607369606567040 20260222.0978 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:11:38.84 +58:43:39.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.97 23:16:40.54 +56:43:17.9
110.16706 -3.78315 galactic Cas Second-epoch detections are separated by 1.2" 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 2009274697096132480 | 23:16:40.33 +56:43:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 40.54 +56 43 17.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009274697096132480,2461093.5978,10.97,0.05,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 2009274697096132480 20260222.0978 10.97CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:40.54 +56:43:17.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.95 23:06:27.75 +55:38:39.4
108.44086 -4.24592 galactic Cas Second-epoch detections are separated by 1.1" 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 2008818434130073088 | 23:06:27.28 +55:38:34.1 (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!
TCP 2026 02 22.0978* 23 06 27.75 +55 38 39.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008818434130073088,2461093.5978,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2008818434130073088 20260222.0978 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:27.75 +55:38:39.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.05 23:18:50.93 +55:58:43.7
110.18512 -4.58446 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J349.7089+55.9868 | 23:18:51.77 +55:58:43.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 50.93 +55 58 43.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.7089+55.9868,2461093.5978,11.05,0.05,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
ATO J349.7089+55.9868 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:50.93 +55:58:43.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 04 18.86 +58 31 23.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2013261285739804800,2461093.5978,10.98,0.05,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
Gaia DR3 2013261285739804800 20260222.0978 10.98CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:04:18.86 +58:31:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 09 39.51 +53 10 14.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0857 Cas,2461093.5978,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0857 Cas 20260222.0978 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:09:39.51 +53:10:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 56 58.44 +56 44 52.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0731 Cas,2461093.5978,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0731 Cas 20260222.0978 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:58.44 +56:44:52.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.02 23:07:37.82 +58:37:21.9
109.75613 -1.56801 galactic Cas Second-epoch detections are separated by 5.9" 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 2010286144715997184 | 23:07:38.68 +58:37:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1928AnHar.100...49C HD 240191
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 07 37.82 +58 37 21.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010286144715997184,2461093.5978,11.02,0.05,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
Gaia DR3 2010286144715997184 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:37.82 +58:37:21.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.02 23:06:31.34 +55:43:26.8
108.48021 -4.17589 galactic Cas Second-epoch detections are separated by 1.4" 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 | ATO J346.6237+55.7314 | 23:06:30.35 +55:43:22.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 31.34 +55 43 26.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.6237+55.7314,2461093.5978,11.02,0.05,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
ATO J346.6237+55.7314 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:31.34 +55:43:26.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.04 23:09:21.89 +55:50:10.1
108.89303 -4.22833 galactic Cas Second-epoch detections are separated by 3.9" 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 2008803728161192576 | 23:09:22.77 +55:50:07.5 (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!
TCP 2026 02 22.0978* 23 09 21.89 +55 50 10.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008803728161192576,2461093.5978,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2008803728161192576 20260222.0978 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:21.89 +55:50:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.05 23:03:47.41 +57:54:28.8
109.00887 -2.02406 galactic Cas 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 2010178804890327424 | 23:03:48.70 +57:54:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 03 47.41 +57 54 28.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010178804890327424,2461093.5978,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2010178804890327424 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:03:47.41 +57:54:28.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.12 23:14:10.23 +52:32:51.6
108.30116 -7.53902 galactic And Second-epoch detections are separated by 0.6" 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 | ATO J348.5559+52.5408 | 23:14:10.51 +52:32:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 10.23 +52 32 51.6 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.5559+52.5408,2461093.5978,11.12,0.05,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
ATO J348.5559+52.5408 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:10.23 +52:32:51.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.13 23:22:12.29 +49:05:33.2
108.25236 -11.21909 galactic And Second-epoch detections are separated by 1.4" 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 1942842818717035776 | 23:22:12.90 +49:05:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S TYC 3644-1705-1
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 22 12.29 +49 05 33.2 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942842818717035776,2461093.5978,11.13,0.05,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 1942842818717035776 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:12.29 +49:05:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 29.74 +53 42 18.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995578149466933376,2461093.5978,11.09,0.05,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 1995578149466933376 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:29.74 +53:42:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 44 32.33 +56 34 50.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Z Cas,2461093.5978,11.23,0.05,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
Z Cas 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:44:32.33 +56:34:50.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.11 23:12:27.51 +53:25:44.3
108.39088 -6.62516 galactic Cas Second-epoch detections are separated by 5.5" 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 1995569971849282048 | 23:12:29.17 +53:25:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 27.51 +53 25 44.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995569971849282048,2461093.5978,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995569971849282048 20260222.0978 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:27.51 +53:25:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 03 35.33 +58 18 40.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010254911712961280,2461093.5978,11.12,0.05,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 2010254911712961280 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:03:35.33 +58:18:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.21 23:25:54.43 +49:05:43.4
108.83513 -11.42112 galactic And Second-epoch detections are separated by 8.5" and 3.1 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 | ATO J351.4905+49.0980 | 23:25:55.02 +49:05:56.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1958PMcCO..13b....V AG+48 2065
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 25 54.43 +49 05 43.4 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.4905+49.0980,2461093.5978,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.4905+49.0980 20260222.0978 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:54.43 +49:05:43.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.18 23:30:05.03 +55:03:39.8
111.38676 -5.97667 galactic Cas Second-epoch detections are separated by 4.3" 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 1997436152321664896 | 23:30:04.25 +55:03:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 30 05.03 +55 03 39.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997436152321664896,2461093.5978,11.18,0.05,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 1997436152321664896 20260222.0978 11.18CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:30:05.03 +55:03:39.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.17 23:16:31.99 +55:54:09.8
109.85396 -4.54045 galactic Cas Second-epoch detections are separated by 1.1" 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 | Large-amplitude variable Gaia DR2 1997148045909494656 | 23:16:33.04 +55:54:10.4 (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: A2V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 31.99 +55 54 09.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1997148045909494656,2461093.5978,11.17,0.05,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
Large-amplitude variable Gaia DR2 1997148045909494656 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:31.99 +55:54:09.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.14 23:10:30.86 +58:26:14.0
110.03235 -1.88403 galactic Cas Second-epoch detections are separated by 1.1" 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 | ATO J347.6115+58.4389 | 23:10:31.96 +58:26:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1955IzKry..14....3B [B55b] 1470
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 10 30.86 +58 26 14.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.6115+58.4389,2461093.5978,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.6115+58.4389 20260222.0978 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:10:30.86 +58:26:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.14 23:05:43.15 +57:00:23.8
108.88609 -2.95397 galactic Cas 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 | ATO J346.4331+56.9938 | 23:05:44.15 +57:00:22.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 05 43.15 +57 00 23.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.4331+56.9938,2461093.5978,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.4331+56.9938 20260222.0978 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:05:43.15 +57:00:23.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.18 23:08:32.89 +56:01:01.2
108.85719 -4.01734 galactic Cas Second-epoch detections are separated by 2.7" 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 2008833896012541440 | 23:08:33.88 +56:01:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1928AnHar.100...49C HD 240197
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 32.89 +56 01 01.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008833896012541440,2461093.5978,11.18,0.05,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 2008833896012541440 20260222.0978 11.18CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:32.89 +56:01:01.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.17 23:08:52.06 +57:47:52.1
109.58655 -2.39164 galactic Cas Second-epoch detections are separated by 1.1" 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 2009992472030712192 | 23:08:53.39 +57:47:49.1 (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!
TCP 2026 02 22.0978* 23 08 52.06 +57 47 52.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009992472030712192,2461093.5978,11.17,0.05,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 2009992472030712192 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:52.06 +57:47:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 23 12.12 +49 02 28.4 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.5978,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.0978 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:23:12.12 +49:02:28.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.12 23:09:27.13 +55:23:03.3
108.73022 -4.65024 galactic Cas Second-epoch detections are separated by 0.9" 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 1996746930328927744 | 23:09:27.80 +55:22:59.5 (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!
TCP 2026 02 22.0978* 23 09 27.13 +55 23 03.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996746930328927744,2461093.5978,11.12,0.05,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 1996746930328927744 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:27.13 +55:23:03.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.24 23:20:02.84 +49:36:34.6
108.10014 -10.61208 galactic And Second-epoch detections are separated by 5.5" 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 1942738816090384000 | 23:20:03.30 +49:36:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1928MeUpp..37....1S BD+48 4002
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 20 02.84 +49 36 34.6 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942738816090384000,2461093.5978,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1942738816090384000 20260222.0978 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:02.84 +49:36:34.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.24 23:12:15.28 +55:01:59.5
108.96769 -5.12676 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J348.0671+55.0458 | 23:12:15.91 +55:02:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 15.28 +55 01 59.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.0671+55.0458,2461093.5978,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.0671+55.0458 20260222.0978 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:15.28 +55:01:59.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.24 23:11:40.79 +56:27:41.9
109.43036 -3.77242 galactic Cas 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 | ATO J347.9115+56.4732 | 23:11:40.57 +56:27:57.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 11 40.79 +56 27 41.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.9115+56.4732,2461093.5978,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.9115+56.4732 20260222.0978 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:11:40.79 +56:27:41.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.21 23:10:02.71 +58:41:25.2
110.07207 -1.62668 galactic Cas Second-epoch detections are separated by 0.6" 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 | Gaia DR3 2010649430226263296 | 23:10:04.39 +58:41:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1928AnHar.100...49C HD 240209
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 10 02.71 +58 41 25.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010649430226263296,2461093.5978,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2010649430226263296 20260222.0978 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:10:02.71 +58:41:25.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 04 02.47 +58 13 01.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230401.08+581303.3,2461093.5978,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J230401.08+581303.3 20260222.0978 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:04:02.47 +58:13:01.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.31 23:13:28.54 +55:16:55.7
109.22326 -4.96070 galactic Cas Second-epoch detections are separated by 2.3" 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 1996707176110755840 | 23:13:28.84 +55:16:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 28.54 +55 16 55.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996707176110755840,2461093.5978,11.31,0.05,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
Gaia DR3 1996707176110755840 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:28.54 +55:16:55.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.34 23:18:56.94 +56:15:28.5
110.29643 -4.32797 galactic Cas Second-epoch detections are separated by 0.1" 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 1997185360590497152 | 23:18:57.75 +56:15:27.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 (LAMOST DR5) J-Ks=1.534+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 56.94 +56 15 28.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997185360590497152,2461093.5978,11.34,0.05,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
Gaia DR3 1997185360590497152 20260222.0978 11.34CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:56.94 +56:15:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.26 23:16:28.99 +53:45:30.8
109.07189 -6.53835 galactic Cas Second-epoch detections are separated by 1.1" 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 | ATO J349.1140+53.7600 | 23:16:30.15 +53:45:33.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 28.99 +53 45 30.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.1140+53.7600,2461093.5978,11.26,0.05,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
ATO J349.1140+53.7600 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:28.99 +53:45:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.29 23:13:33.98 +53:34:16.3
108.59815 -6.55466 galactic Cas Second-epoch detections are separated by 4.2" 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 1995573094286898944 | 23:13:35.10 +53:34:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 33.98 +53 34 16.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995573094286898944,2461093.5978,11.29,0.05,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 1995573094286898944 20260222.0978 11.29CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:33.98 +53:34:16.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 19 32.10 +56 13 42.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997182611810846592,2461093.5978,11.31,0.05,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
Gaia DR3 1997182611810846592 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:19:32.10 +56:13:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.31 23:16:26.88 +58:49:08.5
110.89142 -1.81425 galactic Cas Second-epoch detections are separated by 0.7" 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 2010434029026668288 | 23:16:27.82 +58:49:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1935BSD...C01....0S BSD 19- 38
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 16 26.88 +58 49 08.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010434029026668288,2461093.5978,11.31,0.05,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
Gaia DR3 2010434029026668288 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:16:26.88 +58:49:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.20 23:18:09.24 +52:58:29.7
109.02377 -7.35928 galactic And Second-epoch detections are separated by 4.2" 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 1995660372318029312 | 23:18:09.88 +52:58:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 09.24 +52 58 29.7 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995660372318029312,2461093.5978,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995660372318029312 20260222.0978 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:09.24 +52:58:29.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.34 23:13:38.06 +56:48:20.0
109.80866 -3.55340 galactic Cas Second-epoch detections are separated by 0.8" 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 2009265072067995904 | 23:13:37.85 +56:48:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 38.06 +56 48 20.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009265072067995904,2461093.5978,11.34,0.05,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
Gaia DR3 2009265072067995904 20260222.0978 11.34CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:38.06 +56:48:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 07 07.11 +56 00 24.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 26022,2461093.5978,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 26022 20260222.0978 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:07.11 +56:00:24.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 08 42.25 +55 33 08.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008762732690160384,2461093.5978,11.34,0.05,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
Gaia DR3 2008762732690160384 20260222.0978 11.34CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:42.25 +55:33:08.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.35 23:07:37.72 +55:44:19.8
108.62963 -4.22347 galactic Cas Second-epoch detections are separated by 0.7" 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 2008825752754644864 | 23:07:37.98 +55:44:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8III (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 07 37.72 +55 44 19.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008825752754644864,2461093.5978,11.35,0.05,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 2008825752754644864 20260222.0978 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:37.72 +55:44:19.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.38 23:13:43.83 +53:17:38.1
108.51748 -6.82123 galactic Cas Second-epoch detections are separated by 5.3" 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 1995366630920519040 | 23:13:44.54 +53:17:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=2.093+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 43.83 +53 17 38.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995366630920519040,2461093.5978,11.38,0.05,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
Gaia DR3 1995366630920519040 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:43.83 +53:17:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 00.25 +51 10 32.8 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991946977953827968,2461093.5978,11.18,0.05,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 1991946977953827968 20260222.0978 11.18CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:00.25 +51:10:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 04.20 +54 28 23.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996469303643437824,2461093.5978,11.43,0.05,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 1996469303643437824 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:04.20 +54:28:23.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 11 52.99 +53 32 26.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995598765311057664,2461093.5978,11.39,0.05,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
Gaia DR3 1995598765311057664 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:11:52.99 +53:32:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.44 23:14:56.39 +55:55:22.1
109.65251 -4.44090 galactic Cas 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 1997162064686230784 | 23:14:56.94 +55:55:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 56.39 +55 55 22.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997162064686230784,2461093.5978,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997162064686230784 20260222.0978 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:56.39 +55:55:22.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 06 57.04 +54 57 57.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996730845667836416,2461093.5978,11.40,0.05,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 1996730845667836416 20260222.0978 11.40CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:06:57.04 +54:57:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 17 05.82 +55 40 24.9 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997082521890803584,2461093.5978,11.39,0.05,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
Gaia DR3 1997082521890803584 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:05.82 +55:40:24.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 18 47.71 +53 46 04.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995757812237333504,2461093.5978,11.43,0.05,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 1995757812237333504 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:18:47.71 +53:46:04.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.45 23:09:25.64 +53:47:19.3
108.11009 -6.12152 galactic Cas Second-epoch detections are separated by 2.5" 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 | ATO J347.3463+53.7921 | 23:09:26.39 +53:47:20.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 09 25.64 +53 47 19.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.3463+53.7921,2461093.5978,11.45,0.05,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
ATO J347.3463+53.7921 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:25.64 +53:47:19.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.49 23:14:28.64 +52:51:44.6
108.46183 -7.26366 galactic And Second-epoch detections are separated by 5.6" 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 | ATO J348.6225+52.8737 | 23:14:29.53 +52:51:46.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+52 1734
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 14 28.64 +52 51 44.6 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.6225+52.8737,2461093.5978,11.49,0.05,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
ATO J348.6225+52.8737 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:28.64 +52:51:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.49 23:09:59.02 +53:37:49.1
108.12527 -6.29938 galactic Cas Second-epoch detections are separated by 3.1" 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 1995609038872679680 | 23:09:59.62 +53:37:42.1 (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!
TCP 2026 02 22.0978* 23 09 59.02 +53 37 49.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995609038872679680,2461093.5978,11.49,0.05,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 1995609038872679680 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:59.02 +53:37:49.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.52 23:15:33.51 +58:28:46.6
110.66110 -2.08921 galactic Cas 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 2010407503308555776 | 23:15:34.59 +58:28:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1955IzKry..14....3B [B55b] 1892
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 15 33.51 +58 28 46.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010407503308555776,2461093.5978,11.52,0.05,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 2010407503308555776 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:15:33.51 +58:28:46.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.49 23:05:11.38 +56:14:55.1
108.51722 -3.62046 galactic Cas 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 | ATO J346.3140+56.2528 | 23:05:12.67 +56:14:55.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B BD+55 2892
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 05 11.38 +56 14 55.1 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.3140+56.2528,2461093.5978,11.49,0.05,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
ATO J346.3140+56.2528 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:05:11.38 +56:14:55.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 33 47.54 +53 41 03.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1454 Cas,2461093.5978,11.59,0.05,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
V1454 Cas 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:33:47.54 +53:41:03.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 21 20.40 +51 21 41.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0859 Cas,2461093.5978,11.78,0.05,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
V0859 Cas 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:21:20.40 +51:21:41.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 30.61 +54 23 54.0 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996423089793917824,2461093.5978,11.51,0.05,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 1996423089793917824 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:30.61 +54:23:54.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 12 19.26 +53 42 43.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J231220.11+534301.5,2461093.5978,11.60,0.05,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
ZTF J231220.11+534301.5 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:19.26 +53:42:43.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 13 15.27 +52 46 41.3 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995293719555319296,2461093.5978,11.57,0.05,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 1995293719555319296 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:13:15.27 +52:46:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 21 17.63 +56 04 44.1 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2321166+560444,2461093.5978,11.69,0.05,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
NSVS J2321166+560444 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:17.63 +56:04:44.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.73 23:43:12.33 +57:41:43.0
113.89065 -3.97376 galactic Cas Second-epoch detections are separated by 1.6" 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 1998682173872613248 | 23:43:10.02 +57:41:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 43 12.33 +57 41 43.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998682173872613248,2461093.5978,11.73,0.05,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
Gaia DR3 1998682173872613248 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:43:12.33 +57:41:43.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 15 11.49 +53 51 44.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J231512.71+535148.9,2461093.5978,11.68,0.05,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
ASASSN-V J231512.71+535148.9 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:15:11.49 +53:51:44.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 11.74 23:47:11.25 +56:01:23.7
113.99164 -5.72920 galactic Cas Second-epoch detections are separated by 8.6" 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 1994911811062195584 | 23:47:12.55 +56:01:52.5 (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!
TCP 2026 02 22.0978* 23 47 11.25 +56 01 23.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994911811062195584,2461093.5978,11.74,0.05,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 1994911811062195584 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:47:11.25 +56:01:23.7 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 47 12.80 +58 54 07.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2347121+585422,2461093.5978,11.77,0.05,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
NSVS J2347121+585422 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:47:12.80 +58:54:07.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 09 19.54 +54 58 17.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CzeV711,2461093.5978,11.64,0.05,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
CzeV711 20260222.0978 11.64CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:19.54 +54:58:17.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 12.27 00:29:48.16 +53:16:48.6
119.65653 -9.45393 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J007.4302+53.2798 | 00:29:48.16 +53:16:48.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 29 48.16 +53 16 48.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.4302+53.2798,2461093.5978,12.27,0.05,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
ATO J007.4302+53.2798 20260222.0978 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:48.16 +53:16:48.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 56 48.42 +53 24 18.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235648.52+532416.2,2461093.5978,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J235648.52+532416.2 20260222.0978 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:48.42 +53:24:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 07 55.85 +53 01 06.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1559200,2461093.5978,11.16,0.05,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
NSVS 1559200 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:07:55.85 +53:01:06.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 00 51.65 +56 11 55.1 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J000051.70+561155.7,2461093.5978,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J000051.70+561155.7 20260222.0978 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:00:51.65 +56:11:55.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 59 41.17 +56 24 11.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
QZ Cas,2461093.5978,11.06,0.05,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
QZ Cas 20260222.0978 11.06CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:59:41.17 +56:24:11.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 10 48.25 +57 29 23.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0958 Cas,2461093.5978,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0958 Cas 20260222.0978 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:10:48.25 +57:29:23.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.88 00:05:04.99 +52:22:05.5
115.78030 -9.85870 galactic Cas Second-epoch detections are separated by 0.1" 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 | ATO J001.2649+52.3699 | 00:05:04.37 +52:22:07.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 05 04.99 +52 22 05.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.2649+52.3699,2461093.5978,10.88,0.05,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
ATO J001.2649+52.3699 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:05:04.99 +52:22:05.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 25 47.41 +56 18 54.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J232545.69+561907.9,2461093.5978,10.86,0.05,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
ASASSN-V J232545.69+561907.9 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:25:47.41 +56:18:54.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 53 54.77 +53 12 53.4 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1543541,2461093.5978,10.24,0.05,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 1543541 20260222.0978 10.24CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:53:54.77 +53:12:53.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.0978 2461093.5978 10.72 23:26:29.17 +58:01:45.9
111.85859 -3.00424 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J351.6250+58.0188 | 23:26:29.78 +58:01:46.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K 1928AnHar.100...49C HD 240298
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 26 29.17 +58 01 45.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.6250+58.0188,2461093.5978,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.6250+58.0188 20260222.0978 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:26:29.17 +58:01:45.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 05 00.39 +57 39 10.5 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J230459.26+573910.8,2461093.5978,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J230459.26+573910.8 20260222.0978 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:05:00.39 +57:39:10.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-10-02_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 27 35.59 +55 43 18.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DG Cas,2461093.5978,11.45,0.05,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
DG Cas 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:35.59 +55:43:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 37 38.97 +53 07 18.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0849 Cas,2461093.5978,10.88,0.05,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
V0849 Cas 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:37:38.97 +53:07:18.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 39 57.42 +56 10 19.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J233956.81+561020.9,2461093.5978,11.59,0.05,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
ASASSN-V J233956.81+561020.9 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:39:57.42 +56:10:19.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 15 18.29 +53 11 56.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419244578251557888,2461093.5978,10.53,0.05,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 419244578251557888 20260222.0978 10.53CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:15:18.29 +53:11:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 51 56.51 +54 48 08.2 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J235156.25+544809.4,2461093.5978,10.40,0.05,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
ZTF J235156.25+544809.4 20260222.0978 10.40CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:51:56.51 +54:48:08.2 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 54 23.12 +53 19 24.0 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235423.05+531920.6,2461093.5978,9.21,0.05,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 J235423.05+531920.6 20260222.0978 9.21CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:54:23.12 +53:19:24.0 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 09 36.40 +51 34 03.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SS Cas,2461093.5978,9.66,0.05,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
SS Cas 20260222.0978 9.66CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:09:36.40 +51:34:03.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 38 10.33 +56 01 45.5 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LS Cas,2461093.5978,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LS Cas 20260222.0978 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:38:10.33 +56:01:45.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 35 51.01 +58 44 14.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1529950,2461093.5978,10.69,0.05,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
NSVS 1529950 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:35:51.01 +58:44:14.3 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 25 19.46 +54 00 14.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002519.56+540015.2,2461093.5978,11.00,0.05,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
ASASSN-V J002519.56+540015.2 20260222.0978 11.00CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:19.46 +54:00:14.1 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 01 06.96 +52 14 04.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0001073+521359,2461093.5978,10.54,0.05,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
NSVS J0001073+521359 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:01:06.96 +52:14:04.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 03 21.40 +55 40 50.9 7.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Y Cas,2461093.5978,7.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Y Cas 20260222.0978 7.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:03:21.40 +55:40:50.9 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 43 02.08 +52 58 19.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234301.76+525817.2,2461093.5978,10.32,0.05,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
ASASSN-V J234301.76+525817.2 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:43:02.08 +52:58:19.8 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 16 54.67 +57 31 48.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0016550+573153,2461093.5978,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0016550+573153 20260222.0978 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:16:54.67 +57:31:48.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 10 08.98 +54 52 34.5 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TT Cas,2461093.5978,9.04,0.05,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
TT Cas 20260222.0978 9.04CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:10:08.98 +54:52:34.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 09 14.19 +55 08 31.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1559961,2461093.5978,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1559961 20260222.0978 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:09:14.19 +55:08:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 40 53.89 +53 15 41.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2340531+531540,2461093.5978,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2340531+531540 20260222.0978 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:40:53.89 +53:15:41.5 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 23 48 15.12 +56 52 54.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2348147+565257,2461093.5978,11.57,0.05,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 J2348147+565257 20260222.0978 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:48:15.12 +56:52:54.4 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.0978* 00 05 52.54 +55 02 01.6 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FH Cas,2461093.5978,9.84,0.05,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
FH Cas 20260222.0978 9.84CV 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:05:52.54 +55:02:01.6 ;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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20_00sec_-14_90C_LIGHT_0004_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: 2461032.67300796 23.12.2025 04:08:57.888 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461032.67300796 23.12.2025 04:08:57.888 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461093.59812295 22.02.2026 02:21:07.823 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 593
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.71
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: 11 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): 33215
Objects passed selection criteria: 33104
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 26459.2
Average stars matched: 25617.8 (96.8196 %)
Memory usage VmPeak: 135712 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 20:31:00 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: 2461032.67300796 23.12.2025 04:08:57.888 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461032.67300796 23.12.2025 04:08:57.888 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461093.59812295 22.02.2026 02:21:07.823 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3666
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: 231 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): 227433
Objects passed selection criteria: 226765
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 168029
Average stars matched: 160401 (95.4606 %)
Memory usage VmPeak: 2370100 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 20:46:16 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:
Cas-04-Q2b1x1
#######################################
########### Starting Cas-04-Q2b1x1 ###########
Processing Cas-04-Q2b1x1
server tau has sufficient free disk space available: 1148023 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1148023 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.png' -> 'transient_report/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits_preview.png'
Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
renamed 'Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.png' -> 'transient_report/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits_preview.png'
Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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= 634.2293
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 888.8633
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1488.2705
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 798.3713
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1489.1963
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 798.6788
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.34658
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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: 2461093.59754242
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits'
wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits'
wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits'
wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits'
The image scale is 5.91"/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 23:59:29.292 +54:01:34.99
Second-epoch image center 00:00:05.013 +53:59:45.24
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:29.292 +54:01:34.99
Second-epoch image center 00:00:04.099 +54:00:08.18
Angular distance between the image centers 0.09 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 00:00:05.013 +53:59:45.24
Second-epoch second image center 00:00:04.099 +54:00:08.18
Angular distance between the image centers 0.00675 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.k48MhSlLvJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.d2Jg4XWRF9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits &> /tmp/tmp.umLZriRFi2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits &> /tmp/tmp.JuP8rXrowa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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 9303 out of 34682 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.957779
a=0.000000 b=1.000000 c=22.957779
From vast_summary.log: estimated ref. image limiting mag.: -7.71
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 520 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
2.1 pix Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
3.7 pix Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
3.7 pix Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Limiting magnitude estimates:
15.2 mag. Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
15.2 mag. Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
14.3 mag. Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
14.3 mag. Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.8 (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.k48MhSlLvJ (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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4152, passed=34682
Got 34682 stars (including 30470 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 34682 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 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: 1.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.65"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.62"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 968 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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.d2Jg4XWRF9 (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/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4148, passed=34605
Got 34605 stars (including 30412 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 34605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.10"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.02"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.00"
Estimated accuracy of the plate solution: 1.17"
Excluding outliers - 910 stars left (next iteration limit 958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.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.umLZriRFi2 (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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2548, passed=18740
Got 18740 stars (including 16186 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 18740 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 953 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: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.04"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.04"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits -region wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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.JuP8rXrowa (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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2548, passed=18753
Got 18753 stars (including 16203 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 18753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 954 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: 1.07"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.04"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.04"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits -region wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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 Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53111.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 212s
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: 104s
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Considering the candidate 52284_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52284_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52285_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52285_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:21:49.42 +53:49:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.552 419688364325997184 005.45661775895 +53.82571208578 11.9382 11.6334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52286_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52286_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52289_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52289_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:26:00.93 +51:36:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 4.006 1991597092737686016 351.50536158734 +51.61001760637 10.4528 10.0532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52290_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52290_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52292_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52292_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52294_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52294_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:24:59.76 +51:08:42.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52295_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52295_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:55.43 +57:32:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 3.932 2009416461072340608 350.97978213173 +57.53419206862 10.4067 9.9483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52296_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52296_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:54.91 +53:38:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 3.970 1995567119991276288 348.73065094145 +53.63646992278 10.0030 9.3695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52297_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52297_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:30:06.92 +49:41:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.306 1942939614399826688 352.52860498803 +49.69311311921 10.2068 9.8041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52299_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52299_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:42.65 +52:55:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.772 1992622456050856576 350.42743675457 +52.92285858890 10.3337 9.8604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52300_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52300_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:21.75 +56:44:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 2.246 1997292799187223808 350.84176232081 +56.74387766144 10.3439 9.7283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52302_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52302_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:16.66 +57:06:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.657 1997336096761761408 351.31871382307 +57.10299306346 10.3051 9.8347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52303_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52303_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:32:24.07 +58:49:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 4.708 2011184102113196544 353.09857781007 +58.82478900379 10.2431 9.7614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52304_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52304_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:18.91 +51:56:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 3.377 1992337064064189696 350.32987180811 +51.94504950357 10.2167 9.7875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52305_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52305_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:00.84 +52:50:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.126 1992610808099754752 350.75352002999 +52.84232835537 10.2644 9.7936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52306_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52306_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:22:48.96 +52:41:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.081 1992606169535165056 350.70396723506 +52.68945041442 10.2734 9.7841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52307_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52307_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52308_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52308_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:27:40.28 +58:24:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.536 2011145516126582144 351.91718076285 +58.40432817800 10.1515 9.6906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52310_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52310_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:50.36 +50:52:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 2.892 1991280085492665984 350.95974792504 +50.87078193458 10.1029 9.4669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52311_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52311_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:32:28.08 +58:17:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 1.429 2010918466977410432 353.11774672312 +58.29647564627 10.2818 9.8290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52313_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52313_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:34.26 +52:29:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 3.302 1992632179857478400 349.39406499176 +52.48971953082 10.0164 9.5500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52314_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52314_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:31.22 +54:18:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 3.001 1995880824401808128 351.38116848103 +54.31565370855 10.5997 10.2911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52315_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52315_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:32:09.14 +48:58:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 4.283 1942099273980226816 353.03985395394 +48.97500482485 9.9627 9.5490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52317_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52317_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:04.77 +52:50:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 5.534 1992646851465920128 349.76791119298 +52.83838364278 9.9733 9.5375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52320_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52320_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:46.45 +50:49:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 0.536 1991127390813882112 349.19346000661 +50.82022141053 9.6076 9.2374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52321_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52321_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:10.35 +53:40:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 3.115 1995568941057400960 348.79445236526 +53.67908309578 10.1761 9.4073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52322_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52322_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:01.46 +53:41:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 5.090 1995753727721537408 349.25841665742 +53.69588464297 9.8666 9.4421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52324_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52324_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52327_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52327_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:29:27.77 +58:25:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.083 2010961760248615424 352.36656937188 +58.42638299976 9.9792 9.4886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52328_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52328_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:27:05.16 +56:40:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 4.514 1997256553966269696 351.77053747496 +56.67485923442 10.3060 10.0496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52329_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52329_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:22.91 +53:40:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.801 1995720604939780864 350.34724082337 +53.67393626798 10.0302 9.6107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52330_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52330_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:03.59 +50:45:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 5.100 1991277822049540352 350.76349885539 +50.75403654836 9.7324 9.3571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52331_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52331_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:51.41 +52:46:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 4.987 1995293135437419392 348.46545812067 +52.78108913230 9.7252 9.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52332_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52332_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:31.88 +54:02:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 5.017 1996010635493328256 348.88071696882 +54.04378592734 9.7494 9.4078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52333_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52333_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:22:18.83 +53:44:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 3.350 1995722494725650432 350.57913700713 +53.73685492225 10.0112 9.6453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52334_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52334_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52335_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52335_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:22:48.72 +52:07:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 3.899 1992339984641926400 350.70174656353 +52.12923764099 9.8366 9.5293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52337_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52337_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:25.50 +57:10:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 2.366 1997337333705115648 351.35505010980 +57.16946195102 10.0012 9.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52338_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52338_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52339_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52339_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:32:04.42 +57:48:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 3.752 1998883826872353664 353.01662286643 +57.80841575574 10.0838 9.6935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52340_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52340_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:35.71 +51:14:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 1.043 1991388288607493632 351.39861696908 +51.24900951670 9.9625 9.5335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52341_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52341_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:30:32.24 +50:50:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 5.074 1943288468823436288 352.63603104528 +50.84427625105 10.0903 9.6563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52344_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52344_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:24:37.53 +57:07:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 3.225 1997336887035703936 351.15472930185 +57.11943561209 9.9430 9.5419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52346_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52346_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52347_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52347_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:41.54 +56:55:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 5.223 2009317165728980480 350.17051565114 +56.91937480258 9.7204 9.2115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52348_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52348_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:04.61 +53:21:24.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)
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Considering the candidate 52350_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52350_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52351_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52351_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 52352_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52352_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:48.82 +55:43:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.921 1996921576577099008 349.95447802286 +55.72290978922 9.7169 9.1805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52353_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52353_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52354_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52354_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:24:24.29 +56:41:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.742 1997311495189038336 351.10033461480 +56.69772995495 9.7284 9.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52355_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52355_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:05.95 +51:46:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 4.098 1992352594665300992 349.77478073039 +51.77963941577 9.6466 9.1766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52356_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52356_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:24.32 +51:52:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 0.623 1992332940895049344 350.35142548565 +51.88186438089 9.6210 9.1629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52357_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52357_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52358_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52358_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:47.03 +54:43:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 5.157 1996058700464266624 350.19359521420 +54.72431420454 9.7459 9.6276 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#
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Considering the candidate 52359_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52359_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52360_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52360_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:40.20 +54:17:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 2.087 1995879892385797760 351.41848889243 +54.29722107705 9.8688 9.5302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52361_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52361_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52362_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52362_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52364_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52364_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 52365_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52365_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 52366_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52366_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 52368_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52368_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52369_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52369_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:25:57.93 +52:51:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 2.386 1992517688910645888 351.49028015125 +52.85939648403 9.6433 9.2724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52372_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52372_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52373_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52373_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52374_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52374_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:24:15.19 +56:30:55.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52375_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52375_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52377_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52377_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:45.13 +49:01:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52378_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52378_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:33.20 +49:24:29.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52379_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52379_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:30:01.89 +58:33:00.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52381_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52381_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:41.85 +53:12:40.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52382_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52382_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:44.08 +48:16:59.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52383_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52383_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:23.81 +57:10:12.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52385_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52385_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:56:12.08 +57:59:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52386_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52386_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:14.08 +50:37:02.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52387_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52387_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:24:07.27 +57:32:08.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52388_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52388_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:29:51.45 +58:33:00.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52391_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52391_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:08.85 +57:26:55.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52393_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52393_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:22.65 +50:46:09.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52394_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52394_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:53.66 +56:41:28.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52397_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52397_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:06.68 +48:54:59.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52398_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52398_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:06.40 +53:03:28.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52400_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52400_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:50.39 +57:38:55.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52402_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52402_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:53.40 +56:32:11.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52403_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52403_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:19.64 +50:29:16.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52404_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52404_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:06.83 +57:57:11.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52405_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52405_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52406_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52406_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:50.80 +56:40:35.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52407_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52407_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:42.19 +58:02:35.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52409_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52409_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:23.36 +57:10:47.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52412_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52412_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:08.97 +56:50:50.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52415_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52415_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:29.92 +57:01:45.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52416_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52416_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:38.88 +55:42:33.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52417_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52417_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:22:08.25 +49:31:50.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52418_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52418_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:31.01 +55:11:24.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52420_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52420_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:30.59 +55:05:21.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52421_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52421_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:11.67 +51:34:27.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52424_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52424_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:40.50 +51:53:07.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52425_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52425_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:38.91 +56:32:37.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52427_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52427_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:06.58 +53:47:15.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52428_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52428_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52430_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52430_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52432_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52432_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:35.50 +56:54:05.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52433_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52433_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:20.25 +58:31:02.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52435_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52435_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:12.40 +52:20:54.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52436_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52436_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:17.78 +55:48:26.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52437_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52437_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:40.59 +56:09:11.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52438_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52438_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:04.51 +57:27:34.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52441_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52441_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:53.49 +57:50:13.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52443_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52443_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:12.35 +52:48:50.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52445_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52445_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:57.67 +56:00:07.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52446_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52446_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:11.32 +54:32:32.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52448_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52448_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:40.99 +50:44:14.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52450_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52450_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:28.32 +58:10:01.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52451_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52451_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:27.26 +54:36:04.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52452_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52452_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:58.50 +54:56:31.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52453_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52453_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52454_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52454_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:53.83 +56:43:53.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52455_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52455_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:34.71 +57:05:30.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52457_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52457_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:58.23 +50:27:12.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52458_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52458_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:11.35 +58:14:35.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52459_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52459_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:04.05 +48:50:54.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52460_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52460_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:51.92 +56:14:00.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52461_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52461_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:01.07 +53:20:28.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52462_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52462_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52463_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52463_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:19.68 +49:43:11.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52464_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52464_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:05.00 +53:11:32.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52466_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52466_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:12.71 +54:24:17.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.86, MAG_FAINT_SEARCH_LIMIT=10.84)
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Considering the candidate 52468_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52468_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:47.21 +51:28:44.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52469_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52469_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52470_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52470_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52471_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52471_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52473_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52473_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:23.91 +53:40:19.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52474_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52474_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52475_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52475_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:50.69 +52:22:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.01, MAG_FAINT_SEARCH_LIMIT=10.99)GAIADR2_OUTPUT=# 3.472 1995243863571783936 347.95969612595 +52.37235989022 8.7863 8.1292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52478_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52478_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52482_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52482_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:29.09 +55:25:38.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52483_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52483_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:10.29 +49:13:46.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52484_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52484_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:44.67 +53:55:56.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52485_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52485_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:34.55 +52:18:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 1.824 1992580193571952768 349.39478439629 +52.30326125507 9.2658 9.2105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52487_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52487_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:35.77 +48:50:17.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52488_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52488_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:58.27 +56:56:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.08, MAG_FAINT_SEARCH_LIMIT=11.06)GAIADR2_OUTPUT=# 3.764 2009458006296729344 348.24089132076 +56.94430398958 8.8325 7.8912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52489_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52489_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52490_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52490_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:24.58 +54:51:00.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52495_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52495_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:35.33 +58:21:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.12, MAG_FAINT_SEARCH_LIMIT=11.10)GAIADR2_OUTPUT=# 2.267 2010438117833406208 349.89648164024 +58.35669562755 8.9664 8.2419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52496_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52496_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:26.48 +54:25:31.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52497_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52497_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:15.43 +53:34:26.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52498_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52498_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:34.46 +58:47:09.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52499_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52499_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:44.23 +55:43:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.11, MAG_FAINT_SEARCH_LIMIT=11.09)GAIADR2_OUTPUT=# 1.408 1996780705951969408 347.93359855257 +55.72328227239 8.9333 8.3688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52500_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52500_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:51.55 +50:06:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 1.299 1991175120790882944 350.21522375599 +50.11073118150 9.3359 9.2981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52501_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52501_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52502_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52502_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:46.29 +55:17:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.15, MAG_FAINT_SEARCH_LIMIT=11.13)GAIADR2_OUTPUT=# 2.594 1996751220996170496 347.94199487984 +55.29806560696 8.9761 8.2739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52503_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52503_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52504_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52504_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52505_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52505_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52506_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52506_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52507_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52507_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:44.26 +56:39:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.19, MAG_FAINT_SEARCH_LIMIT=11.17)GAIADR2_OUTPUT=# 1.596 2009261777833458816 348.18361023422 +56.65668470622 8.9598 8.2173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52508_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52508_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:45.11 +54:26:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.25, MAG_FAINT_SEARCH_LIMIT=11.23)GAIADR2_OUTPUT=# 3.628 1996034343712893952 349.18964222820 +54.43934936760 9.4218 9.3530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52509_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52509_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:00.52 +58:28:04.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52510_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52510_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:18.72 +50:01:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 3.219 1990836123311546496 349.07908963664 +50.02791740583 9.1244 8.9178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52513_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52513_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52514_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52514_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:09.80 +54:34:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 3.611 1996042143373427968 349.29252445551 +54.56687908684 9.4033 9.3452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52515_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52515_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:28.54 +49:14:31.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52516_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52516_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52517_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52517_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52518_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52518_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:27.80 +58:24:51.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52519_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52519_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:25.66 +55:48:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 2.837 1996782870615873024 348.10632129382 +55.80249121288 9.1657 8.9128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52521_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52521_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:44.14 +57:06:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 5.388 2009521503094718464 347.93657390039 +57.10885304242 9.0167 8.7433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52523_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52523_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:54.46 +58:06:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 4.998 2010384791520667776 347.72950469218 +58.10834225551 8.9935 8.6947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52524_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52524_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:27.43 +56:43:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 0.770 2009125232234629248 346.61467537418 +56.71918389400 8.7674 8.0287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52525_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52525_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:17.47 +57:51:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 2.268 2009580288304220672 349.07393374151 +57.86308313052 9.1715 8.9339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52526_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52526_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52529_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52529_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:29.39 +57:29:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 5.530 2009545073875351040 348.11982030578 +57.48522950340 8.9740 7.9204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52530_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52530_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:47.00 +57:31:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.28, MAG_FAINT_SEARCH_LIMIT=11.26)GAIADR2_OUTPUT=# 0.301 2010298960892610432 347.69595763322 +57.52739392620 8.9085 7.9688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52531_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52531_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:04.59 +56:23:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 4.726 2009205427861821056 349.27146683708 +56.39687500543 9.2706 9.0267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52534_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52534_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52535_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52535_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52536_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52536_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52537_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52537_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52539_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52539_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:30.31 +53:02:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 2.941 1995534753116823936 347.37519995514 +53.04440223658 9.0386 8.3172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52540_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52540_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:03:56.33 +58:13:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 4.802 2010250857263897472 345.98704166655 +58.22250852412 8.8223 8.1696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52541_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52541_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:43.23 +57:37:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 3.894 2010303152781181440 348.17850384787 +57.61825608303 9.0579 8.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52542_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52542_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:03.05 +54:40:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 4.373 1996486758390405120 348.01471430837 +54.67108396105 9.3370 9.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52543_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52543_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52545_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52545_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52548_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52548_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52549_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52549_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:30.10 +54:58:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 4.231 1996500227408034560 348.37711810527 +54.97354066067 9.2204 8.9411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52550_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52550_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52551_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52551_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:15.25 +56:13:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 0.886 2008874303065252352 347.31310977725 +56.22672388826 9.1007 8.3152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52553_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52553_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:09.08 +56:20:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 3.095 2008867774715328256 348.03903576126 +56.33829011579 9.3511 9.1668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52554_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52554_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:56.32 +54:43:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 2.041 1996479164888595584 348.48549635793 +54.73075216984 9.3581 9.1614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52559_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52559_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:07.93 +55:23:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 2.997 1997072454487279872 348.78449065622 +55.39081933532 9.4939 8.9581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52560_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52560_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:05.17 +52:37:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 2.561 1995230257117340032 347.27269526709 +52.61979141725 9.3047 9.2218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52561_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52561_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52562_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52562_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52564_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52564_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:02.62 +57:04:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.44, MAG_FAINT_SEARCH_LIMIT=11.42)GAIADR2_OUTPUT=# 1.090 2009893825219464192 346.26143884584 +57.07593845563 8.9165 8.0715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52566_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52566_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52567_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52567_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52568_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52568_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:16.92 +49:50:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 5.628 1991155604459588224 350.06812134223 +49.84153142373 9.2295 8.7002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52569_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52569_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52570_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52570_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52571_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52571_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:38.01 +54:05:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 4.751 1996388730054960256 347.65650093229 +54.09704687021 9.3532 8.6242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52572_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52572_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52573_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52573_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:02.38 +58:39:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 3.516 2010600948634261632 347.75811572863 +58.65649837009 9.0154 7.8269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52576_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52576_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:22.88 +48:58:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 2.509 1990732189405228288 348.59629339112 +48.98050744382 9.1507 8.7399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52577_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52577_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52579_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52579_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:34.62 +56:58:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 3.240 2009469997845366784 348.14588728402 +56.97217142570 9.3009 8.9494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52581_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52581_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:29.28 +57:21:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 3.237 2009533597722858240 348.37033335782 +57.35501681210 9.6532 9.1947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52582_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52582_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52583_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52583_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52585_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52585_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:57.34 +54:19:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 4.356 1996454146694884736 346.99096839171 +54.32692983395 9.4107 9.3025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52586_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52586_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:02.64 +49:51:29.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)
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Considering the candidate 52589_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52589_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52590_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52590_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52591_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52591_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:35.46 +56:44:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.56, MAG_FAINT_SEARCH_LIMIT=11.54)GAIADR2_OUTPUT=# 4.337 2009263805058016256 348.39988397544 +56.73810370253 9.5325 9.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52592_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52592_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:28.63 +52:33:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 3.439 1995307772686854016 347.62085999259 +52.56560643464 9.4710 9.3576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52593_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52593_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52594_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52594_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:09.53 +49:59:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 2.570 1991021189163382400 348.54068574193 +49.99786674138 9.4225 9.1789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52595_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52595_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:09.63 +54:18:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 2.880 1996396323557378688 347.79137582934 +54.30394991653 9.4962 9.4322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52600_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52600_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:48.13 +57:08:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 2.896 2009475392324199296 348.19910378544 +57.13472327368 9.3610 8.5488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52601_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52601_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:57.81 +52:50:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 2.589 1995327525236380800 347.74202938696 +52.84910089995 9.6537 9.5252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52602_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52602_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52603_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52603_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:55.07 +52:44:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 3.087 1995327873133403264 347.47996961760 +52.73608928778 9.3843 8.8008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52604_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52604_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:30.63 +49:01:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 5.149 1942695076141115264 348.87977513956 +49.03226979857 9.4762 9.3791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52605_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52605_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:43.38 +52:44:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)
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Considering the candidate 52606_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52606_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52607_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52607_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52608_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52608_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52610_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52610_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:24.87 +58:07:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 4.919 2009646675618937344 350.85619628323 +58.12326487119 9.6992 9.3765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52612_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52612_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:38.45 +54:40:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 2.838 1996803623894160256 348.91141774207 +54.67894162500 9.7795 9.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52613_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52613_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52614_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52614_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52616_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52616_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52617_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52617_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52619_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52619_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:07.27 +49:07:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 3.391 1942699268029625088 349.28152888111 +49.12745380902 9.5556 9.3037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52620_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52620_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:20.26 +58:15:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 2.020 2010392694260858240 348.08352156095 +58.26488869017 9.4014 8.6207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52621_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52621_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52622_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52622_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:39.42 +58:49:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 4.826 2010469213396964608 350.16677221673 +58.81697493642 9.6319 8.8893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52623_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52623_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52624_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52624_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:48.52 +54:19:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 2.197 1996416905041013504 348.20318372711 +54.33027269374 9.6943 9.4266 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 52625_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52625_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:59.96 +55:45:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)
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Considering the candidate 52626_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52626_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52627_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52627_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:37.87 +54:26:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 1.932 1996421543605614208 348.15769444718 +54.43697823051 9.4140 8.9530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52628_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52628_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52632_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52632_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52635_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52635_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:44.89 +57:57:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 4.334 2010191621074073984 346.93885773656 +57.95986151367 9.1962 8.6059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52636_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52636_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:23:13.16 +58:08:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 5.758 2009645507388145152 350.80759343269 +58.13522904968 9.8697 9.5271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52637_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52637_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52638_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52638_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52639_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52639_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52640_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52640_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:02.35 +57:09:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 3.590 2009150452283652992 347.76159544411 +57.15822249405 9.4360 9.0196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52641_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52641_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52644_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52644_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52646_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52646_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:34.81 +58:29:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 4.973 2010278688652442112 346.39728725978 +58.49113225169 9.1376 8.2987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52647_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52647_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52649_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52649_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:06.95 +53:27:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.321 1995594642142144512 347.52801662503 +53.46232029383 9.5686 8.8420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52650_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52650_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52651_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52651_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:49.94 +49:02:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.232 414614912737207808 011.45901897638 +49.03841002597 10.1445 9.0759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52652_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52652_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:49.48 +55:49:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 4.979 1997143785305470592 348.70817552623 +55.82578380577 9.8713 9.6918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52654_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52654_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:05:36.57 +58:00:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 3.002 2010183924491789824 346.40363747594 +58.00391865571 9.2939 8.4691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52655_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52655_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:11.07 +56:39:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 1.977 2009229995068926464 349.54676690367 +56.66327361257 9.9564 9.7564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52656_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52656_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:51.20 +52:27:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 5.298 1992259892094802176 348.96529335255 +52.45694314989 10.0653 9.9013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52657_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52657_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:58.42 +54:44:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 5.161 1996713189065529856 346.74538856224 +54.74676722031 9.5095 9.3037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52658_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52658_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:02.09 +57:07:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 3.786 2009477934944907392 348.50692949656 +57.13372264795 9.6142 8.6452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52659_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52659_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52660_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52660_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52661_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52661_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:53.85 +48:50:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 3.573 1942688547790860672 348.72587015788 +48.84698189877 9.5677 9.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52662_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52662_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52663_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52663_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:48.79 +55:39:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.523 1997140551191294336 348.45243255145 +55.66379943202 9.7342 8.9541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52666_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52666_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:08.11 +57:05:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 2.707 2009887399948690432 346.53391590116 +57.09858442363 9.3779 8.5562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52667_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52667_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:37.60 +57:14:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 2.433 2009490991646255872 348.90711027657 +57.23381266342 9.7699 9.3869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52668_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52668_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:06.82 +58:08:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 5.330 2010379053444433024 348.02585206805 +58.14940624420 9.4798 8.5090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52669_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52669_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52670_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52670_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 52671_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52671_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:57.87 +56:22:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 5.471 2009064552935796224 347.24381170654 +56.37549555330 9.6415 9.3413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52673_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52673_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:21.00 +54:30:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 3.300 1996463565566275584 347.33873617132 +54.50851294421 9.7161 9.5357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52674_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52674_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:03.10 +57:46:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.865 2009567682583967360 349.51331539503 +57.77702715758 9.8531 9.5281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52676_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52676_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52680_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52680_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:37.13 +56:27:59.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)
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Considering the candidate 52681_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52681_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:17.82 +51:32:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 1.573 1992298890388360064 349.57424929989 +51.53882577679 9.6947 9.2736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52682_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52682_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52684_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52684_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:42.08 +54:52:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 1.206 1996858462038406144 348.67478320444 +54.86905708141 9.8943 9.3633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52685_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52685_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:08.76 +55:23:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 3.634 1996712192632404352 348.28805192975 +55.39609099027 9.8499 9.5632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52686_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52686_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:03.14 +56:59:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 4.194 2009153544660102400 347.26129317445 +56.98619246696 9.5493 8.6598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52687_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52687_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52688_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52688_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:26.52 +55:11:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.326 1996704839648530816 348.11161459554 +55.19836304247 9.7863 9.4686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52691_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52691_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:14.49 +49:26:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 3.517 1990713703864237824 348.31187067101 +49.43656479578 9.6729 9.4878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52692_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52692_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52694_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52694_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52696_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52696_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52699_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52699_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52701_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52701_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52704_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52704_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52705_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52705_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52706_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52706_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52708_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52708_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:08.45 +55:09:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 2.136 1996702468826497920 347.78418960662 +55.15919887508 9.7469 8.8716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52710_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52710_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52711_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52711_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52712_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52712_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:13.99 +58:14:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 4.419 2010250994702854528 346.05992664304 +58.24520775738 9.3136 8.4175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52713_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52713_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:42.78 +56:56:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 1.478 2009284936298335488 349.67760242725 +56.93795905287 10.0812 9.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52714_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52714_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52715_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52715_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:39.22 +52:51:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 5.868 1995517229650128768 347.41554027823 +52.85318803197 9.9409 9.7841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52716_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52716_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:21.21 +58:13:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 4.746 2010576342762840192 347.59072618994 +58.23279657944 9.6875 9.3770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52718_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52718_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52719_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52719_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:55.42 +56:24:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 3.883 2008883064798748800 347.72901989897 +56.41624997893 9.7521 8.9767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52720_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52720_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:37.19 +49:32:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 3.592 1990728444191923200 348.15466606527 +49.54377050586 9.3923 8.8183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52721_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52721_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:05.38 +52:57:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 5.306 1995332030661873280 347.77464611146 +52.96710765513 10.1016 10.0454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52722_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52722_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52726_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52726_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:22.69 +52:57:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.108 1995336905444950400 347.84533964877 +52.96569328388 9.6968 9.3278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52729_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52729_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52730_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52730_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:46.59 +54:52:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 2.847 1996856602313123456 348.94470935661 +54.87314543992 9.9646 9.5436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52731_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52731_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:11.20 +55:42:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 5.116 2008784589787119488 347.79882747168 +55.70623901886 9.9254 9.6494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52732_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52732_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:30:28.23 +57:51:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.572 2010873249561360000 352.61745714166 +57.85185022081 10.0691 9.6242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52734_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52734_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52736_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52736_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52737_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52737_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:04:57.09 +57:47:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 4.185 2010167706695052672 346.23571306133 +57.79557160070 9.4784 8.5254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52738_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52738_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:43.91 +55:43:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)
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Considering the candidate 52740_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52740_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52743_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52743_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52744_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52744_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52745_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52745_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:04.42 +56:09:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.585 2009176256443524608 348.52114251544 +56.16298446583 10.0617 9.9214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52746_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52746_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52747_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52747_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52748_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52748_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:19.01 +56:15:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.684 2009041703709344512 346.82786909309 +56.25518773813 9.6602 8.7607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52751_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52751_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:52.21 +54:56:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.104 1996497135031630976 348.46733340534 +54.93873343516 10.1128 9.6764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52752_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52752_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:28.72 +55:34:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.452 1997136707199457280 348.37117902899 +55.57703810711 10.0580 9.7350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52753_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52753_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52755_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52755_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:59.64 +55:17:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 3.634 1997070560404255616 348.49992465410 +55.29295454516 10.1591 9.9961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52756_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52756_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:31.75 +58:40:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.678 2010428492807378816 349.13416159500 +58.66654770343 9.9341 9.1580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52759_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52759_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:20.34 +56:43:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.796 2009133719090912000 347.08453560502 +56.71892381579 9.7345 8.8969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52760_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52760_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:17.46 +53:00:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 4.435 1995338004956574336 347.82453496162 +52.99978552435 10.0675 9.9440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52761_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52761_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52762_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52762_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:34.70 +56:08:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 4.879 2009172683030782976 348.64622389549 +56.14000055144 10.2363 9.8674 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 52763_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52763_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52764_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52764_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:20.20 +57:18:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.022 2009504048346789120 348.83564624551 +57.30774264773 10.0706 9.8195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52766_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52766_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:01.29 +53:32:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 2.592 1995609451189312512 347.25656860267 +53.53371042702 9.8166 9.3579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52767_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52767_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52768_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52768_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:19.86 +53:35:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 2.809 1995610172743812480 347.33164102621 +53.58449801116 9.8536 9.1023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52771_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52771_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:04.90 +57:44:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 5.089 2009610597894003072 350.02088699594 +57.73985889425 10.1966 9.7422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52773_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52773_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:29.00 +52:36:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.601 1995308696095240448 347.87247924855 +52.60518149775 10.1134 9.9883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52774_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52774_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:41.17 +48:59:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 3.241 1942693942269736064 348.67127465378 +48.98592247592 9.6003 8.9761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52776_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52776_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52777_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52777_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52780_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52780_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52781_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52781_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:41.98 +58:02:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 5.360 2009670246398978688 350.17742586221 +58.04385440817 10.0838 9.6243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52782_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52782_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:25.60 +58:19:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.251 2010360808422552704 349.10732803256 +58.32121167265 9.9491 9.4362 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 52783_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52783_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:18.36 +53:23:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 1.383 1995548565731835392 347.82609754005 +53.39217210005 10.0493 9.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52784_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52784_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52785_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52785_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52787_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52787_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52788_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52788_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:22.29 +49:08:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 2.557 1942701707570979072 349.09372892025 +49.14370011931 9.9223 9.4970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52789_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52789_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:09.22 +56:23:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.232 2009053626538311040 346.53836503322 +56.38603560908 9.7917 8.9703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52790_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52790_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:27.86 +54:51:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 4.806 1996659209915407488 347.61769116993 +54.85426031239 10.1188 9.9140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52792_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52792_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52793_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52793_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52794_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52794_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:55.03 +55:01:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 4.559 1996720984421311488 346.97989058460 +55.01958669051 9.8274 9.3289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52797_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52797_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52798_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52798_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52799_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52799_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:50:40.15 +53:33:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.322 1993449696812004352 357.66723155600 +53.55302899875 10.3057 8.7937 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52800_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52800_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:20:59.85 +49:25:33.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)
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Considering the candidate 52801_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52801_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:02.19 +57:35:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 2.201 2009561326032030976 348.75965891537 +57.60045708491 10.2017 9.3066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52802_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52802_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:24.22 +49:24:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.760 1990767854812690688 349.35165727414 +49.41258312960 10.3205 10.1500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52804_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52804_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:06.08 +58:25:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.615 425150982916596224 011.02559328377 +58.42185313748 10.8755 10.1306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52807_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52807_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:14.24 +55:29:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.763 1997078914118093952 349.06161495566 +55.49060616101 10.2023 9.8200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52809_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52809_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52810_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52810_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52811_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52811_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52815_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52815_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:19.94 +53:21:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.590 1995590037928343680 347.58427814091 +53.36201494684 10.0473 9.5818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52816_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52816_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52819_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52819_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52820_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52820_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52821_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52821_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52822_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52822_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52823_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52823_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:32.45 +48:48:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 0.652 1942630239315465984 349.38547068995 +48.80094548899 10.2102 9.8746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52825_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52825_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:19.85 +57:46:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 4.095 2010308272382080128 348.33081598056 +57.78238651380 10.0051 9.0956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52826_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52826_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52827_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52827_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52828_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52828_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52830_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52830_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:19:43.04 +57:31:48.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)
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Considering the candidate 52834_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52834_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:24.38 +57:56:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 3.795 2010325452250998272 348.10010484167 +57.94020370259 9.9952 9.1748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52836_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52836_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:32.99 +55:54:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 3.560 1997159247187615744 348.38570254591 +55.91370785423 10.1899 9.7695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52837_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52837_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:14:58.04 +53:15:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.504 419247086512438528 003.74344618498 +53.25000947936 9.9704 8.4038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52842_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52842_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:08.34 +50:16:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 4.907 1991007891944858624 348.03520690175 +50.28105745605 9.7467 9.1547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52844_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52844_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:39.03 +56:55:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.590 2009469649949647616 348.16380843805 +56.93134965461 10.2772 9.7923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52846_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52846_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:29.92 +54:54:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 4.577 1996815581083335680 349.12576282858 +54.91746553517 10.5550 10.4234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52847_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52847_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52848_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52848_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52850_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52850_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:15.40 +54:26:21.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)
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Considering the candidate 52851_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52851_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:30.62 +56:39:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.182 2009253668935390336 348.62699575148 +56.65469835985 10.2085 9.5093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52852_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52852_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52854_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52854_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52855_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52855_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52856_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52856_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:14.95 +56:23:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 5.461 2009193642470954496 348.56493876883 +56.38941332592 10.2831 9.9950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52860_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52860_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:09.44 +56:25:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 4.655 2009056169159009792 346.78700406133 +56.42744798029 9.8595 8.9015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52861_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52861_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52865_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52865_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52869_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52869_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:03.88 +58:34:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.554 2010588510409102336 348.26697335636 +58.58143070748 9.9253 8.9634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52870_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52870_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:38.70 +55:00:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 5.452 1996732086921544576 346.66038307995 +55.00409724860 9.8327 9.2665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52871_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52871_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:35.79 +58:22:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.203 2010397912640561280 348.15026201436 +58.38194442815 10.0256 9.5290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52872_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52872_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:44.52 +57:23:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 2.595 2009507690479287936 348.93417130210 +57.38697052668 10.1822 9.6574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52873_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52873_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52875_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52875_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52876_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52876_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:11:12.31 +54:50:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.572 1996679619600377472 347.80152869984 +54.84825209142 10.3929 10.2382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52877_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52877_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:09.37 +56:33:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.704 2009076024785680640 347.54063326446 +56.55801787515 10.1627 9.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52878_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52878_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:23.15 +52:25:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 5.485 1995212596205681280 347.34416307903 +52.42156509792 10.0499 9.3515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52882_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52882_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:37.98 +56:52:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 3.368 2009268409263382272 348.90804205605 +56.86740468809 10.3670 10.0206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52883_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52883_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52888_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52888_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:57:21.42 +58:24:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 5.823 1998443992166092544 359.33858608464 +58.41771866188 10.7676 9.3567 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52889_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52889_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:53.96 +55:44:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 2.036 2008825890193606400 346.97476754607 +55.74101886343 9.9842 9.1724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52891_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52891_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:44.56 +49:10:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 4.614 1942711534456234752 349.43456232322 +49.17649645459 10.0510 9.4073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52893_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52893_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:28.58 +56:46:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 5.337 2009126366105947264 346.62178790972 +56.77589977672 9.9630 9.4743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52897_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52897_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:30.49 +52:30:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.420 1995216856819506688 347.37768536731 +52.51026752969 10.2183 9.7752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52898_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52898_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:09.36 +49:58:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 4.148 1990843824194441856 349.29013505712 +49.97116911590 10.4232 10.2273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52899_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52899_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52900_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52900_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52907_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52907_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52908_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52908_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52910_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52910_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52915_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52915_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:31.20 +54:53:29.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)
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Considering the candidate 52916_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52916_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 52918_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52918_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:21.48 +57:36:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.609 2009515352700942976 349.58925064645 +57.60762910636 10.4231 9.9302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52919_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52919_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52920_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52920_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:12:01.16 +55:13:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.577 420583920849447296 003.00560061908 +55.22567458793 10.9187 9.6004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52921_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52921_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52922_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52922_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52925_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52925_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52927_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52927_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:37.37 +57:11:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 5.110 2009478931377641984 348.65333597347 +57.18757397465 10.2588 9.4393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52928_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52928_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:36.17 +55:27:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 5.094 1996747961121070720 347.39832885467 +55.45004641497 10.1641 9.2120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52933_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52933_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:06:25.56 +55:27:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 4.796 2008768715587533312 346.60882582484 +55.46036529498 10.1869 9.7437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52934_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52934_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52935_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52935_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52939_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52939_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:21:13.22 +57:19:56.9 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 52942_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52942_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:22.46 +55:08:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.532 1996693466575257344 348.34477793125 +55.14780285315 10.4741 10.1701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52945_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52945_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:15.62 +49:28:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 3.735 1990804203118663552 348.56609497488 +49.47583631837 10.1620 9.6770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52947_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52947_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:09:09.50 +57:46:51.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)
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Considering the candidate 52948_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52948_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:57:32.99 +55:47:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.876 1994715543933182592 359.38692387732 +55.79057347237 11.2607 9.8440 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52950_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52950_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:18:43.05 +49:55:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.168 1990798675498749696 349.67975535447 +49.91798415573 10.4846 10.0440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52951_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52951_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52952_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52952_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:16:49.69 +51:16:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 5.633 1991919284005360512 349.20945248955 +51.27508366590 11.0322 10.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52955_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52955_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52956_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52956_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52957_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52957_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52959_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52959_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52960_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52960_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:10:17.99 +53:53:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 4.891 1996374608202644992 347.57309255205 +53.89836838755 10.3152 9.4890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52961_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52961_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52963_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52963_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52964_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52964_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:15:55.58 +50:14:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 5.242 1991030500652889472 348.98335765541 +50.24119875646 10.4430 10.0900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52965_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52965_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:57.19 +54:58:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.973 1996497375549783424 348.48966058667 +54.97005162003 10.6294 10.4590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52970_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52970_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:14:27.57 +49:42:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 4.069 1990823242710460544 348.61410507277 +49.71004074696 10.2293 9.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52972_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52972_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:06:19.65 +53:01:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.771 396182665451938048 001.58226330285 +53.01851152084 10.9264 9.5581 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52975_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52975_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:07:48.77 +55:09:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 5.723 1996734900115344128 346.95293432336 +55.15474854915 10.3620 9.9603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52977_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52977_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:22:32.06 +51:21:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 4.024 394867615181682176 005.63474594465 +51.35617781453 11.3457 10.1216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52980_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52980_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 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 52981_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52981_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:52:16.32 +54:38:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.170 1993756396137985664 358.06797605382 +54.64673256581 11.5938 10.1235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52982_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52982_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:14.29 +52:53:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.280 416443675447414400 008.81049211611 +52.89192540241 12.1077 10.5918 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52986_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52986_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52987_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52987_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:18:33.20 +53:39:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.019 419317725833864704 004.63927343172 +53.65407532145 10.8849 9.5700 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52988_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52988_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:08:22.67 +54:48:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 2.093 1996667799849641344 347.09542035884 +54.81111967695 10.2842 9.8544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52989_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52989_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:08:55.47 +57:03:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.391 422342417901130240 002.23161277998 +57.06258103755 10.7575 9.3845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52990_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52990_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52992_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52992_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:09:22.46 +57:39:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.502 422454293209143936 002.34424325694 +57.65682088316 12.0531 10.2457 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52995_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52995_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 52998_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 52998_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:12:42.58 +48:51:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.012 1990639692987673984 348.17773187937 +48.86467556820 10.1966 9.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53000_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53000_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:54:05.13 +53:42:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 3.781 1945510856704617088 358.52196833855 +53.71476019583 11.3160 10.0871 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53001_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53001_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:13:23.55 +54:39:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 5.090 1996477309462739584 348.35054652849 +54.65514159385 10.6606 10.5808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53008_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53008_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53010_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53010_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:24:12.35 +53:51:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.544 419511278541302656 006.05129108682 +53.86219789282 11.9266 11.4562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53013_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53013_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53015_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53015_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53019_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53019_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:04:28.79 +54:36:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.310 420310760923641344 001.12057399811 +54.60457752344 11.2244 9.7801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53025_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53025_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 23:17:25.17 +49:54:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.823 1990841006695962368 349.35560739944 +49.90646189621 10.4704 10.0230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53026_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53026_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53036_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53036_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:21:41.36 +50:53:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.100 394754601704913536 005.42279344157 +50.88641076387 11.5545 10.4241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53039_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53039_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53049_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53049_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:16:09.65 +55:24:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.274 419924248232498432 004.04132087215 +55.40662995610 11.0994 9.6501 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53051_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53051_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:16:25.04 +54:33:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.499 419779834252531072 004.10409416190 +54.55997438951 12.0839 11.6344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53056_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53056_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:49:53.04 +58:13:40.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)
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Considering the candidate 53061_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53061_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:16:06.71 +53:12:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.986 419242585386835200 004.02841045895 +53.21156900336 12.0594 11.3145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53066_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53066_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:34:22.12 +53:44:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.566 416507172252661376 008.59241725842 +53.74733670654 11.8915 11.0679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53075_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53075_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:47.79 +58:27:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.578 425131500943877248 010.69747734901 +58.46258848279 11.8585 11.5757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53076_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53076_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:23:35.19 +54:17:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.234 419628342168257792 005.89654113781 +54.28567959235 12.3042 11.9210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53077_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53077_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:45.17 +54:39:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.376 417963372321435648 009.93978094653 +54.66429930697 11.1515 9.7590 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53078_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53078_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:24:51.74 +54:17:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.339 419622363573908608 006.21542775340 +54.28791361139 12.2092 11.8379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53092_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53092_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:32:25.50 +53:22:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.510 416516071425904128 008.10605219360 +53.37611592849 12.2081 11.8057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53094_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53094_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:31:32.14 +54:36:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.899 418114623896697216 007.88482724691 +54.60368281052 11.9284 10.9315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53101_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53101_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:30:41.90 +50:38:29.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 53111_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 53111_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 53115_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53115_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:24:31.51 +52:47:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.417 419058034926258944 006.13133758069 +52.78522366080 12.4401 11.9369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53119_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
The candidate 53119_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 00:34:02.31 +53:47:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.469 416510470787522176 008.50974040159 +53.78388863834 12.2425 11.6033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20398_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 20398_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 21221_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 21221_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 10305_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 10305_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 09622_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 09622_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 05377_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 05377_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 23465_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 23465_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 10043_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 10043_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 20873_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 20873_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 04246_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 04246_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 51287_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 51287_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 12314_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 12314_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 21567_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 21567_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 10825_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 10825_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 20208_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 20208_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 15602_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 15602_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 20595_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 20595_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 25799_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 25799_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 11313_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 11313_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 02057_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 02057_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 16807_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 16807_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 24027_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 24027_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 11990_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 11990_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 21964_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 21964_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 04962_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 04962_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 14508_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 14508_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 13784_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 13784_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 21123_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 21123_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 08150_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 08150_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 14196_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 14196_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 335s
Prepared the HTML report for the field Cas-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 ####
23:35:51.01 +58:44:14.3
23:26:29.17 +58:01:45.9
00:16:54.67 +57:31:48.6
00:10:48.25 +57:29:23.4
23:48:15.12 +56:52:54.4
23:59:41.17 +56:24:11.1
23:25:47.41 +56:18:54.2
00:00:51.65 +56:11:55.1
23:39:57.42 +56:10:19.5
23:38:10.33 +56:01:45.5
00:03:21.40 +55:40:50.9
23:27:35.59 +55:43:18.0
00:09:14.19 +55:08:31.2
00:05:52.54 +55:02:01.6
00:10:08.98 +54:52:34.5
23:51:56.51 +54:48:08.2
00:25:19.46 +54:00:14.1
00:15:18.29 +53:11:56.7
23:56:48.42 +53:24:18.7
23:54:23.12 +53:19:24.0
23:53:54.77 +53:12:53.4
23:40:53.89 +53:15:41.5
00:07:55.85 +53:01:06.0
23:37:38.97 +53:07:18.8
23:43:02.08 +52:58:19.8
00:05:04.99 +52:22:05.5
00:01:06.96 +52:14:04.4
00:09:36.40 +51:34:03.6
23:05:00.39 +57:39:10.5
23:16:48.90 +54:33:26.6
23:24:26.64 +50:09:59.2
23:15:58.43 +52:22:28.7
23:26:12.57 +54:32:12.5
23:33:18.60 +49:25:54.1
23:28:56.01 +57:57:15.8
23:24:03.02 +57:21:01.3
23:28:22.33 +49:35:07.3
23:25:18.02 +56:06:27.5
23:21:43.73 +50:16:58.3
23:26:51.31 +50:08:05.1
23:06:21.65 +57:32:45.6
23:08:16.74 +56:18:24.7
23:08:10.63 +58:15:54.3
23:23:34.51 +49:16:56.8
23:14:29.46 +51:30:48.1
23:14:32.26 +53:17:07.5
23:31:50.68 +58:46:18.2
23:18:07.49 +54:06:43.0
23:16:51.50 +51:00:45.1
23:36:09.46 +58:47:01.4
23:22:44.87 +48:59:09.0
23:18:33.86 +54:23:59.2
23:23:13.06 +57:09:34.0
23:10:55.86 +53:27:56.6
23:18:45.44 +51:22:46.1
00:15:50.31 +57:32:36.7
23:25:05.09 +58:25:07.5
23:15:50.84 +52:57:36.9
23:06:19.18 +57:19:32.8
23:04:39.84 +58:34:38.4
23:30:07.22 +49:12:19.0
23:12:38.78 +53:54:03.1
23:16:03.91 +52:59:24.8
23:18:09.27 +58:40:45.9
23:19:41.13 +53:03:08.3
23:11:44.96 +51:11:15.3
23:23:32.54 +57:39:03.3
23:21:09.78 +49:01:55.5
23:08:32.28 +53:33:12.4
23:21:27.78 +58:22:08.2
23:20:24.77 +55:31:27.0
23:06:36.13 +57:42:22.9
23:29:47.18 +58:29:35.6
23:23:31.53 +49:00:05.7
23:16:00.21 +50:50:51.8
23:08:41.17 +58:18:06.9
23:12:25.34 +53:51:03.9
23:20:44.78 +57:52:27.7
00:44:42.32 +48:36:30.5
23:06:53.84 +56:42:52.0
23:26:31.38 +49:29:39.6
23:12:22.31 +52:05:19.2
23:12:00.28 +54:37:16.0
23:14:14.19 +49:05:42.7
23:11:30.90 +50:56:33.5
23:07:09.31 +58:33:17.4
23:08:43.94 +55:52:27.8
23:15:16.53 +55:01:21.9
23:37:40.16 +58:50:41.5
23:20:10.60 +58:47:09.3
23:19:32.11 +49:23:44.2
23:10:52.61 +50:48:05.3
23:12:29.99 +50:52:36.3
23:03:33.01 +57:59:54.1
23:08:26.67 +55:49:47.7
23:19:53.05 +56:57:33.3
23:34:48.15 +58:51:33.3
23:21:30.88 +57:53:52.7
23:22:03.16 +58:13:01.6
23:11:38.84 +58:43:39.5
23:16:40.54 +56:43:17.9
23:06:27.75 +55:38:39.4
23:18:50.93 +55:58:43.7
23:04:18.86 +58:31:23.9
00:09:39.51 +53:10:14.8
23:56:58.44 +56:44:52.7
23:07:37.82 +58:37:21.9
23:06:31.34 +55:43:26.8
23:09:21.89 +55:50:10.1
23:03:47.41 +57:54:28.8
23:14:10.23 +52:32:51.6
23:22:12.29 +49:05:33.2
23:13:29.74 +53:42:18.1
23:44:32.33 +56:34:50.2
23:12:27.51 +53:25:44.3
23:03:35.33 +58:18:40.4
23:25:54.43 +49:05:43.4
23:30:05.03 +55:03:39.8
23:16:31.99 +55:54:09.8
23:10:30.86 +58:26:14.0
23:05:43.15 +57:00:23.8
23:08:32.89 +56:01:01.2
23:08:52.06 +57:47:52.1
23:23:12.12 +49:02:28.4
23:09:27.13 +55:23:03.3
23:20:02.84 +49:36:34.6
23:12:15.28 +55:01:59.5
23:11:40.79 +56:27:41.9
23:10:02.71 +58:41:25.2
23:04:02.47 +58:13:01.6
23:13:28.54 +55:16:55.7
23:18:56.94 +56:15:28.5
23:16:28.99 +53:45:30.8
23:13:33.98 +53:34:16.3
23:19:32.10 +56:13:42.5
23:16:26.88 +58:49:08.5
23:18:09.24 +52:58:29.7
23:13:38.06 +56:48:20.0
23:07:07.11 +56:00:24.8
23:08:42.25 +55:33:08.2
23:07:37.72 +55:44:19.8
23:13:43.83 +53:17:38.1
23:12:00.25 +51:10:32.8
23:12:04.20 +54:28:23.8
23:11:52.99 +53:32:26.3
23:14:56.39 +55:55:22.1
23:06:57.04 +54:57:57.2
23:17:05.82 +55:40:24.9
23:18:47.71 +53:46:04.8
23:09:25.64 +53:47:19.3
23:14:28.64 +52:51:44.6
23:09:59.02 +53:37:49.1
23:15:33.51 +58:28:46.6
23:05:11.38 +56:14:55.1
23:33:47.54 +53:41:03.9
00:21:20.40 +51:21:41.6
23:13:30.61 +54:23:54.0
23:12:19.26 +53:42:43.8
23:13:15.27 +52:46:41.3
23:21:17.63 +56:04:44.1
23:43:12.33 +57:41:43.0
23:15:11.49 +53:51:44.7
23:47:11.25 +56:01:23.7
23:47:12.80 +58:54:07.1
23:09:19.54 +54:58:17.4
00:29:48.16 +53:16:48.6
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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits exists and is non-empty
The image scale is 5.91"/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 23:59:29.292 +54:01:34.99
Second-epoch image center 00:00:05.013 +53:59:45.24
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:29.292 +54:01:34.99
Second-epoch image center 00:00:04.099 +54:00:08.18
Angular distance between the image centers 0.09 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 00:00:05.013 +53:59:45.24
Second-epoch second image center 00:00:04.099 +54:00:08.18
Angular distance between the image centers 0.00675 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/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.e1f0TbTlhc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.mh9GONNSTH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits &> /tmp/tmp.BMufgK9m2G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits &> /tmp/tmp.NpNzjZURZj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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 9667 out of 244953 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.810836
a=0.000000 b=1.000000 c=22.810836
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3249 candidate transients before the final filtering. (Hard limit: 3000)
ERROR Too many candidates before filtering (3249)... Skipping SE run (default.sex.telephoto_lens_vSTL)
wait
############ /tmp/tmp.e1f0TbTlhc (5) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=41249, passed=244894
Got 244894 stars (including 203281 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 244894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 966 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: 1.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.74"
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 966 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.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.mh9GONNSTH (5) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=86, blended=41219, passed=244574
Got 244574 stars (including 202984 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 244574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 881 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: 1.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.73"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.73"
Estimated accuracy of the plate solution: 1.06"
Excluding outliers - 909 stars left (next iteration limit 959)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2025-12-22_22-10-02_20.00sec_-15.00C_LIGHT_0156.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.BMufgK9m2G (5) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=20514, passed=94921
Got 94921 stars (including 74342 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 94921 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.06"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.06"
Estimated accuracy of the plate solution: 1.13"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits -region wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-20-17_20.00sec_-14.90C_LIGHT_0004.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.NpNzjZURZj (5) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.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_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=20759, passed=96116
Got 96116 stars (including 75287 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 96116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 958 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: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.05"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.05"
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cas-04-Q2b1x1_202247_TTUQ2b1x1_22144_jNl4ozgr/Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits -region wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-21_20-21-07_20.00sec_-14.90C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:35:51.01 +58:44:14.3
23:26:29.17 +58:01:45.9
00:16:54.67 +57:31:48.6
00:10:48.25 +57:29:23.4
23:48:15.12 +56:52:54.4
23:59:41.17 +56:24:11.1
23:25:47.41 +56:18:54.2
00:00:51.65 +56:11:55.1
23:39:57.42 +56:10:19.5
23:38:10.33 +56:01:45.5
00:03:21.40 +55:40:50.9
23:27:35.59 +55:43:18.0
00:09:14.19 +55:08:31.2
00:05:52.54 +55:02:01.6
00:10:08.98 +54:52:34.5
23:51:56.51 +54:48:08.2
00:25:19.46 +54:00:14.1
00:15:18.29 +53:11:56.7
23:56:48.42 +53:24:18.7
23:54:23.12 +53:19:24.0
23:53:54.77 +53:12:53.4
23:40:53.89 +53:15:41.5
00:07:55.85 +53:01:06.0
23:37:38.97 +53:07:18.8
23:43:02.08 +52:58:19.8
00:05:04.99 +52:22:05.5
00:01:06.96 +52:14:04.4
00:09:36.40 +51:34:03.6
23:05:00.39 +57:39:10.5
23:16:48.90 +54:33:26.6
23:24:26.64 +50:09:59.2
23:15:58.43 +52:22:28.7
23:26:12.57 +54:32:12.5
23:33:18.60 +49:25:54.1
23:28:56.01 +57:57:15.8
23:24:03.02 +57:21:01.3
23:28:22.33 +49:35:07.3
23:25:18.02 +56:06:27.5
23:21:43.73 +50:16:58.3
23:26:51.31 +50:08:05.1
23:06:21.65 +57:32:45.6
23:08:16.74 +56:18:24.7
23:08:10.63 +58:15:54.3
23:23:34.51 +49:16:56.8
23:14:29.46 +51:30:48.1
23:14:32.26 +53:17:07.5
23:31:50.68 +58:46:18.2
23:18:07.49 +54:06:43.0
23:16:51.50 +51:00:45.1
23:36:09.46 +58:47:01.4
23:22:44.87 +48:59:09.0
23:18:33.86 +54:23:59.2
23:23:13.06 +57:09:34.0
23:10:55.86 +53:27:56.6
23:18:45.44 +51:22:46.1
00:15:50.31 +57:32:36.7
23:25:05.09 +58:25:07.5
23:15:50.84 +52:57:36.9
23:06:19.18 +57:19:32.8
23:04:39.84 +58:34:38.4
23:30:07.22 +49:12:19.0
23:12:38.78 +53:54:03.1
23:16:03.91 +52:59:24.8
23:18:09.27 +58:40:45.9
23:19:41.13 +53:03:08.3
23:11:44.96 +51:11:15.3
23:23:32.54 +57:39:03.3
23:21:09.78 +49:01:55.5
23:08:32.28 +53:33:12.4
23:21:27.78 +58:22:08.2
23:20:24.77 +55:31:27.0
23:06:36.13 +57:42:22.9
23:29:47.18 +58:29:35.6
23:23:31.53 +49:00:05.7
23:16:00.21 +50:50:51.8
23:08:41.17 +58:18:06.9
23:12:25.34 +53:51:03.9
23:20:44.78 +57:52:27.7
00:44:42.32 +48:36:30.5
23:06:53.84 +56:42:52.0
23:26:31.38 +49:29:39.6
23:12:22.31 +52:05:19.2
23:12:00.28 +54:37:16.0
23:14:14.19 +49:05:42.7
23:11:30.90 +50:56:33.5
23:07:09.31 +58:33:17.4
23:08:43.94 +55:52:27.8
23:15:16.53 +55:01:21.9
23:37:40.16 +58:50:41.5
23:20:10.60 +58:47:09.3
23:19:32.11 +49:23:44.2
23:10:52.61 +50:48:05.3
23:12:29.99 +50:52:36.3
23:03:33.01 +57:59:54.1
23:08:26.67 +55:49:47.7
23:19:53.05 +56:57:33.3
23:34:48.15 +58:51:33.3
23:21:30.88 +57:53:52.7
23:22:03.16 +58:13:01.6
23:11:38.84 +58:43:39.5
23:16:40.54 +56:43:17.9
23:06:27.75 +55:38:39.4
23:18:50.93 +55:58:43.7
23:04:18.86 +58:31:23.9
00:09:39.51 +53:10:14.8
23:56:58.44 +56:44:52.7
23:07:37.82 +58:37:21.9
23:06:31.34 +55:43:26.8
23:09:21.89 +55:50:10.1
23:03:47.41 +57:54:28.8
23:14:10.23 +52:32:51.6
23:22:12.29 +49:05:33.2
23:13:29.74 +53:42:18.1
23:44:32.33 +56:34:50.2
23:12:27.51 +53:25:44.3
23:03:35.33 +58:18:40.4
23:25:54.43 +49:05:43.4
23:30:05.03 +55:03:39.8
23:16:31.99 +55:54:09.8
23:10:30.86 +58:26:14.0
23:05:43.15 +57:00:23.8
23:08:32.89 +56:01:01.2
23:08:52.06 +57:47:52.1
23:23:12.12 +49:02:28.4
23:09:27.13 +55:23:03.3
23:20:02.84 +49:36:34.6
23:12:15.28 +55:01:59.5
23:11:40.79 +56:27:41.9
23:10:02.71 +58:41:25.2
23:04:02.47 +58:13:01.6
23:13:28.54 +55:16:55.7
23:18:56.94 +56:15:28.5
23:16:28.99 +53:45:30.8
23:13:33.98 +53:34:16.3
23:19:32.10 +56:13:42.5
23:16:26.88 +58:49:08.5
23:18:09.24 +52:58:29.7
23:13:38.06 +56:48:20.0
23:07:07.11 +56:00:24.8
23:08:42.25 +55:33:08.2
23:07:37.72 +55:44:19.8
23:13:43.83 +53:17:38.1
23:12:00.25 +51:10:32.8
23:12:04.20 +54:28:23.8
23:11:52.99 +53:32:26.3
23:14:56.39 +55:55:22.1
23:06:57.04 +54:57:57.2
23:17:05.82 +55:40:24.9
23:18:47.71 +53:46:04.8
23:09:25.64 +53:47:19.3
23:14:28.64 +52:51:44.6
23:09:59.02 +53:37:49.1
23:15:33.51 +58:28:46.6
23:05:11.38 +56:14:55.1
23:33:47.54 +53:41:03.9
00:21:20.40 +51:21:41.6
23:13:30.61 +54:23:54.0
23:12:19.26 +53:42:43.8
23:13:15.27 +52:46:41.3
23:21:17.63 +56:04:44.1
23:43:12.33 +57:41:43.0
23:15:11.49 +53:51:44.7
23:47:11.25 +56:01:23.7
23:47:12.80 +58:54:07.1
23:09:19.54 +54:58:17.4
00:29:48.16 +53:16:48.6
########### Completed Cas-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 ####
23:16:48.90 +54:33:26.6
23:24:26.64 +50:09:59.2
23:15:58.43 +52:22:28.7
23:26:12.57 +54:32:12.5
23:33:18.60 +49:25:54.1
23:28:56.01 +57:57:15.8
23:24:03.02 +57:21:01.3
23:28:22.33 +49:35:07.3
23:25:18.02 +56:06:27.5
23:21:43.73 +50:16:58.3
23:26:51.31 +50:08:05.1
23:06:21.65 +57:32:45.6
23:08:16.74 +56:18:24.7
23:08:10.63 +58:15:54.3
23:23:34.51 +49:16:56.8
23:14:29.46 +51:30:48.1
23:14:32.26 +53:17:07.5
23:31:50.68 +58:46:18.2
23:18:07.49 +54:06:43.0
23:16:51.50 +51:00:45.1
23:36:09.46 +58:47:01.4
23:22:44.87 +48:59:09.0
23:18:33.86 +54:23:59.2
23:23:13.06 +57:09:34.0
23:10:55.86 +53:27:56.6
23:18:45.44 +51:22:46.1
00:15:50.31 +57:32:36.7
23:25:05.09 +58:25:07.5
23:15:50.84 +52:57:36.9
23:06:19.18 +57:19:32.8
23:04:39.84 +58:34:38.4
23:30:07.22 +49:12:19.0
23:12:38.78 +53:54:03.1
23:16:03.91 +52:59:24.8
23:18:09.27 +58:40:45.9
23:19:41.13 +53:03:08.3
23:11:44.96 +51:11:15.3
23:23:32.54 +57:39:03.3
23:21:09.78 +49:01:55.5
23:08:32.28 +53:33:12.4
23:21:27.78 +58:22:08.2
23:20:24.77 +55:31:27.0
23:06:36.13 +57:42:22.9
23:29:47.18 +58:29:35.6
23:23:31.53 +49:00:05.7
23:16:00.21 +50:50:51.8
23:08:41.17 +58:18:06.9
23:12:25.34 +53:51:03.9
23:20:44.78 +57:52:27.7
00:44:42.32 +48:36:30.5
23:06:53.84 +56:42:52.0
23:26:31.38 +49:29:39.6
23:12:22.31 +52:05:19.2
23:12:00.28 +54:37:16.0
23:14:14.19 +49:05:42.7
23:11:30.90 +50:56:33.5
23:07:09.31 +58:33:17.4
23:08:43.94 +55:52:27.8
23:15:16.53 +55:01:21.9
23:37:40.16 +58:50:41.5
23:20:10.60 +58:47:09.3
23:19:32.11 +49:23:44.2
23:10:52.61 +50:48:05.3
23:12:29.99 +50:52:36.3
23:03:33.01 +57:59:54.1
23:08:26.67 +55:49:47.7
23:19:53.05 +56:57:33.3
23:34:48.15 +58:51:33.3
23:21:30.88 +57:53:52.7
23:22:03.16 +58:13:01.6
23:11:38.84 +58:43:39.5
23:16:40.54 +56:43:17.9
23:06:27.75 +55:38:39.4
23:18:50.93 +55:58:43.7
23:04:18.86 +58:31:23.9
00:09:39.51 +53:10:14.8
23:56:58.44 +56:44:52.7
23:07:37.82 +58:37:21.9
23:06:31.34 +55:43:26.8
23:09:21.89 +55:50:10.1
23:03:47.41 +57:54:28.8
23:14:10.23 +52:32:51.6
23:22:12.29 +49:05:33.2
23:13:29.74 +53:42:18.1
23:44:32.33 +56:34:50.2
23:12:27.51 +53:25:44.3
23:03:35.33 +58:18:40.4
23:25:54.43 +49:05:43.4
23:30:05.03 +55:03:39.8
23:16:31.99 +55:54:09.8
23:10:30.86 +58:26:14.0
23:05:43.15 +57:00:23.8
23:08:32.89 +56:01:01.2
23:08:52.06 +57:47:52.1
23:23:12.12 +49:02:28.4
23:09:27.13 +55:23:03.3
23:20:02.84 +49:36:34.6
23:12:15.28 +55:01:59.5
23:11:40.79 +56:27:41.9
23:10:02.71 +58:41:25.2
23:04:02.47 +58:13:01.6
23:13:28.54 +55:16:55.7
23:18:56.94 +56:15:28.5
23:16:28.99 +53:45:30.8
23:13:33.98 +53:34:16.3
23:19:32.10 +56:13:42.5
23:16:26.88 +58:49:08.5
23:18:09.24 +52:58:29.7
23:13:38.06 +56:48:20.0
23:07:07.11 +56:00:24.8
23:08:42.25 +55:33:08.2
23:07:37.72 +55:44:19.8
23:13:43.83 +53:17:38.1
23:12:00.25 +51:10:32.8
23:12:04.20 +54:28:23.8
23:11:52.99 +53:32:26.3
23:14:56.39 +55:55:22.1
23:06:57.04 +54:57:57.2
23:17:05.82 +55:40:24.9
23:18:47.71 +53:46:04.8
23:09:25.64 +53:47:19.3
23:14:28.64 +52:51:44.6
23:09:59.02 +53:37:49.1
23:15:33.51 +58:28:46.6
23:05:11.38 +56:14:55.1
23:33:47.54 +53:41:03.9
00:21:20.40 +51:21:41.6
23:13:30.61 +54:23:54.0
23:12:19.26 +53:42:43.8
23:13:15.27 +52:46:41.3
23:21:17.63 +56:04:44.1
23:43:12.33 +57:41:43.0
23:15:11.49 +53:51:44.7
23:47:11.25 +56:01:23.7
23:47:12.80 +58:54:07.1
23:09:19.54 +54:58:17.4
00:29:48.16 +53:16:48.6
23:56:48.42 +53:24:18.7
00:07:55.85 +53:01:06.0
00:00:51.65 +56:11:55.1
23:59:41.17 +56:24:11.1
00:10:48.25 +57:29:23.4
00:05:04.99 +52:22:05.5
23:25:47.41 +56:18:54.2
23:53:54.77 +53:12:53.4
23:26:29.17 +58:01:45.9
23:05:00.39 +57:39:10.5
23:27:35.59 +55:43:18.0
23:37:38.97 +53:07:18.8
23:39:57.42 +56:10:19.5
00:15:18.29 +53:11:56.7
23:51:56.51 +54:48:08.2
23:54:23.12 +53:19:24.0
00:09:36.40 +51:34:03.6
23:38:10.33 +56:01:45.5
23:35:51.01 +58:44:14.3
00:25:19.46 +54:00:14.1
00:01:06.96 +52:14:04.4
00:03:21.40 +55:40:50.9
23:43:02.08 +52:58:19.8
00:16:54.67 +57:31:48.6
00:10:08.98 +54:52:34.5
00:09:14.19 +55:08:31.2
23:40:53.89 +53:15:41.5
23:48:15.12 +56:52:54.4
00:05:52.54 +55:02:01.6
###################################################################################
23:16:48.90 +54:33:26.6 -- not an asteroid (will add it to exclusion list)
23:24:26.64 +50:09:59.2 -- not an asteroid (will add it to exclusion list)
23:15:58.43 +52:22:28.7 -- not an asteroid (will add it to exclusion list)
23:26:12.57 +54:32:12.5 -- not an asteroid (will add it to exclusion list)
23:33:18.60 +49:25:54.1 -- not an asteroid (will add it to exclusion list)
23:28:56.01 +57:57:15.8 -- not an asteroid (will add it to exclusion list)
23:24:03.02 +57:21:01.3 -- not an asteroid (will add it to exclusion list)
23:28:22.33 +49:35:07.3 -- not an asteroid (will add it to exclusion list)
23:25:18.02 +56:06:27.5 -- not an asteroid (will add it to exclusion list)
23:21:43.73 +50:16:58.3 -- not an asteroid (will add it to exclusion list)
23:26:51.31 +50:08:05.1 -- not an asteroid (will add it to exclusion list)
23:06:21.65 +57:32:45.6 -- not an asteroid (will add it to exclusion list)
23:08:16.74 +56:18:24.7 -- not an asteroid (will add it to exclusion list)
23:08:10.63 +58:15:54.3 -- not an asteroid (will add it to exclusion list)
23:23:34.51 +49:16:56.8 -- not an asteroid (will add it to exclusion list)
23:14:29.46 +51:30:48.1 -- not an asteroid (will add it to exclusion list)
23:14:32.26 +53:17:07.5 -- not an asteroid (will add it to exclusion list)
23:31:50.68 +58:46:18.2 -- not an asteroid (will add it to exclusion list)
23:18:07.49 +54:06:43.0 -- not an asteroid (will add it to exclusion list)
23:16:51.50 +51:00:45.1 -- not an asteroid (will add it to exclusion list)
23:36:09.46 +58:47:01.4 -- not an asteroid (will add it to exclusion list)
23:22:44.87 +48:59:09.0 -- not an asteroid (will add it to exclusion list)
23:18:33.86 +54:23:59.2 -- not an asteroid (will add it to exclusion list)
23:23:13.06 +57:09:34.0 -- not an asteroid (will add it to exclusion list)
23:10:55.86 +53:27:56.6 -- not an asteroid (will add it to exclusion list)
23:18:45.44 +51:22:46.1 -- not an asteroid (will add it to exclusion list)
00:15:50.31 +57:32:36.7 -- not an asteroid (will add it to exclusion list)
23:25:05.09 +58:25:07.5 -- not an asteroid (will add it to exclusion list)
23:15:50.84 +52:57:36.9 -- not an asteroid (will add it to exclusion list)
23:06:19.18 +57:19:32.8 -- not an asteroid (will add it to exclusion list)
23:04:39.84 +58:34:38.4 -- not an asteroid (will add it to exclusion list)
23:30:07.22 +49:12:19.0 -- not an asteroid (will add it to exclusion list)
23:12:38.78 +53:54:03.1 -- not an asteroid (will add it to exclusion list)
23:16:03.91 +52:59:24.8 -- not an asteroid (will add it to exclusion list)
23:18:09.27 +58:40:45.9 -- not an asteroid (will add it to exclusion list)
23:19:41.13 +53:03:08.3 -- not an asteroid (will add it to exclusion list)
23:11:44.96 +51:11:15.3 -- not an asteroid (will add it to exclusion list)
23:23:32.54 +57:39:03.3 -- not an asteroid (will add it to exclusion list)
23:21:09.78 +49:01:55.5 -- not an asteroid (will add it to exclusion list)
23:08:32.28 +53:33:12.4 -- not an asteroid (will add it to exclusion list)
23:21:27.78 +58:22:08.2 -- not an asteroid (will add it to exclusion list)
23:20:24.77 +55:31:27.0 -- not an asteroid (will add it to exclusion list)
23:06:36.13 +57:42:22.9 -- not an asteroid (will add it to exclusion list)
23:29:47.18 +58:29:35.6 -- not an asteroid (will add it to exclusion list)
23:23:31.53 +49:00:05.7 -- not an asteroid (will add it to exclusion list)
23:16:00.21 +50:50:51.8 -- not an asteroid (will add it to exclusion list)
23:08:41.17 +58:18:06.9 -- not an asteroid (will add it to exclusion list)
23:12:25.34 +53:51:03.9 -- not an asteroid (will add it to exclusion list)
23:20:44.78 +57:52:27.7 -- not an asteroid (will add it to exclusion list)
00:44:42.32 +48:36:30.5 -- not an asteroid (will add it to exclusion list)
23:06:53.84 +56:42:52.0 -- not an asteroid (will add it to exclusion list)
23:26:31.38 +49:29:39.6 -- not an asteroid (will add it to exclusion list)
23:12:22.31 +52:05:19.2 -- not an asteroid (will add it to exclusion list)
23:12:00.28 +54:37:16.0 -- not an asteroid (will add it to exclusion list)
23:14:14.19 +49:05:42.7 -- not an asteroid (will add it to exclusion list)
23:11:30.90 +50:56:33.5 -- not an asteroid (will add it to exclusion list)
23:07:09.31 +58:33:17.4 -- not an asteroid (will add it to exclusion list)
23:08:43.94 +55:52:27.8 -- not an asteroid (will add it to exclusion list)
23:15:16.53 +55:01:21.9 -- not an asteroid (will add it to exclusion list)
23:37:40.16 +58:50:41.5 -- not an asteroid (will add it to exclusion list)
23:20:10.60 +58:47:09.3 -- not an asteroid (will add it to exclusion list)
23:19:32.11 +49:23:44.2 -- not an asteroid (will add it to exclusion list)
23:10:52.61 +50:48:05.3 -- not an asteroid (will add it to exclusion list)
23:12:29.99 +50:52:36.3 -- not an asteroid (will add it to exclusion list)
23:03:33.01 +57:59:54.1 -- not an asteroid (will add it to exclusion list)
23:08:26.67 +55:49:47.7 -- not an asteroid (will add it to exclusion list)
23:19:53.05 +56:57:33.3 -- not an asteroid (will add it to exclusion list)
23:34:48.15 +58:51:33.3 -- not an asteroid (will add it to exclusion list)
23:21:30.88 +57:53:52.7 -- not an asteroid (will add it to exclusion list)
23:22:03.16 +58:13:01.6 -- not an asteroid (will add it to exclusion list)
23:11:38.84 +58:43:39.5 -- not an asteroid (will add it to exclusion list)
23:16:40.54 +56:43:17.9 -- not an asteroid (will add it to exclusion list)
23:06:27.75 +55:38:39.4 -- not an asteroid (will add it to exclusion list)
23:18:50.93 +55:58:43.7 -- not an asteroid (will add it to exclusion list)
23:04:18.86 +58:31:23.9 -- not an asteroid (will add it to exclusion list)
00:09:39.51 +53:10:14.8 -- not an asteroid (will add it to exclusion list)
23:56:58.44 +56:44:52.7 -- not an asteroid (will add it to exclusion list)
23:07:37.82 +58:37:21.9 -- not an asteroid (will add it to exclusion list)
23:06:31.34 +55:43:26.8 -- not an asteroid (will add it to exclusion list)
23:09:21.89 +55:50:10.1 -- not an asteroid (will add it to exclusion list)
23:03:47.41 +57:54:28.8 -- not an asteroid (will add it to exclusion list)
23:14:10.23 +52:32:51.6 -- not an asteroid (will add it to exclusion list)
23:22:12.29 +49:05:33.2 -- not an asteroid (will add it to exclusion list)
23:13:29.74 +53:42:18.1 -- not an asteroid (will add it to exclusion list)
23:44:32.33 +56:34:50.2 -- not an asteroid (will add it to exclusion list)
23:12:27.51 +53:25:44.3 -- not an asteroid (will add it to exclusion list)
23:03:35.33 +58:18:40.4 -- not an asteroid (will add it to exclusion list)
23:25:54.43 +49:05:43.4 -- not an asteroid (will add it to exclusion list)
23:30:05.03 +55:03:39.8 -- not an asteroid (will add it to exclusion list)
23:16:31.99 +55:54:09.8 -- not an asteroid (will add it to exclusion list)
23:10:30.86 +58:26:14.0 -- not an asteroid (will add it to exclusion list)
23:05:43.15 +57:00:23.8 -- not an asteroid (will add it to exclusion list)
23:08:32.89 +56:01:01.2 -- not an asteroid (will add it to exclusion list)
23:08:52.06 +57:47:52.1 -- not an asteroid (will add it to exclusion list)
23:23:12.12 +49:02:28.4 -- not an asteroid (will add it to exclusion list)
23:09:27.13 +55:23:03.3 -- not an asteroid (will add it to exclusion list)
23:20:02.84 +49:36:34.6 -- not an asteroid (will add it to exclusion list)
23:12:15.28 +55:01:59.5 -- not an asteroid (will add it to exclusion list)
23:11:40.79 +56:27:41.9 -- not an asteroid (will add it to exclusion list)
23:10:02.71 +58:41:25.2 -- not an asteroid (will add it to exclusion list)
23:04:02.47 +58:13:01.6 -- not an asteroid (will add it to exclusion list)
23:13:28.54 +55:16:55.7 -- not an asteroid (will add it to exclusion list)
23:18:56.94 +56:15:28.5 -- not an asteroid (will add it to exclusion list)
23:16:28.99 +53:45:30.8 -- not an asteroid (will add it to exclusion list)
23:13:33.98 +53:34:16.3 -- not an asteroid (will add it to exclusion list)
23:19:32.10 +56:13:42.5 -- not an asteroid (will add it to exclusion list)
23:16:26.88 +58:49:08.5 -- not an asteroid (will add it to exclusion list)
23:18:09.24 +52:58:29.7 -- not an asteroid (will add it to exclusion list)
23:13:38.06 +56:48:20.0 -- not an asteroid (will add it to exclusion list)
23:07:07.11 +56:00:24.8 -- not an asteroid (will add it to exclusion list)
23:08:42.25 +55:33:08.2 -- not an asteroid (will add it to exclusion list)
23:07:37.72 +55:44:19.8 -- not an asteroid (will add it to exclusion list)
23:13:43.83 +53:17:38.1 -- not an asteroid (will add it to exclusion list)
23:12:00.25 +51:10:32.8 -- not an asteroid (will add it to exclusion list)
23:12:04.20 +54:28:23.8 -- not an asteroid (will add it to exclusion list)
23:11:52.99 +53:32:26.3 -- not an asteroid (will add it to exclusion list)
23:14:56.39 +55:55:22.1 -- not an asteroid (will add it to exclusion list)
23:06:57.04 +54:57:57.2 -- not an asteroid (will add it to exclusion list)
23:17:05.82 +55:40:24.9 -- not an asteroid (will add it to exclusion list)
23:18:47.71 +53:46:04.8 -- not an asteroid (will add it to exclusion list)
23:09:25.64 +53:47:19.3 -- not an asteroid (will add it to exclusion list)
23:14:28.64 +52:51:44.6 -- not an asteroid (will add it to exclusion list)
23:09:59.02 +53:37:49.1 -- not an asteroid (will add it to exclusion list)
23:15:33.51 +58:28:46.6 -- not an asteroid (will add it to exclusion list)
23:05:11.38 +56:14:55.1 -- not an asteroid (will add it to exclusion list)
23:33:47.54 +53:41:03.9 -- not an asteroid (will add it to exclusion list)
00:21:20.40 +51:21:41.6 -- not an asteroid (will add it to exclusion list)
23:13:30.61 +54:23:54.0 -- not an asteroid (will add it to exclusion list)
23:12:19.26 +53:42:43.8 -- not an asteroid (will add it to exclusion list)
23:13:15.27 +52:46:41.3 -- not an asteroid (will add it to exclusion list)
23:21:17.63 +56:04:44.1 -- not an asteroid (will add it to exclusion list)
23:43:12.33 +57:41:43.0 -- not an asteroid (will add it to exclusion list)
23:15:11.49 +53:51:44.7 -- not an asteroid (will add it to exclusion list)
23:47:11.25 +56:01:23.7 -- not an asteroid (will add it to exclusion list)
23:47:12.80 +58:54:07.1 -- not an asteroid (will add it to exclusion list)
23:09:19.54 +54:58:17.4 -- not an asteroid (will add it to exclusion list)
00:29:48.16 +53:16:48.6 -- not an asteroid (will add it to exclusion list)
23:56:48.42 +53:24:18.7 -- not an asteroid (will add it to exclusion list)
00:07:55.85 +53:01:06.0 -- not an asteroid (will add it to exclusion list)
00:00:51.65 +56:11:55.1 -- not an asteroid (will add it to exclusion list)
23:59:41.17 +56:24:11.1 -- not an asteroid (will add it to exclusion list)
00:10:48.25 +57:29:23.4 -- not an asteroid (will add it to exclusion list)
00:05:04.99 +52:22:05.5 -- not an asteroid (will add it to exclusion list)
23:25:47.41 +56:18:54.2 -- not an asteroid (will add it to exclusion list)
23:53:54.77 +53:12:53.4 -- not an asteroid (will add it to exclusion list)
23:26:29.17 +58:01:45.9 -- not an asteroid (will add it to exclusion list)
23:05:00.39 +57:39:10.5 -- not an asteroid (will add it to exclusion list)
23:27:35.59 +55:43:18.0 -- not an asteroid (will add it to exclusion list)
23:37:38.97 +53:07:18.8 -- not an asteroid (will add it to exclusion list)
23:39:57.42 +56:10:19.5 -- not an asteroid (will add it to exclusion list)
00:15:18.29 +53:11:56.7 -- not an asteroid (will add it to exclusion list)
23:51:56.51 +54:48:08.2 -- not an asteroid (will add it to exclusion list)
23:54:23.12 +53:19:24.0 -- not an asteroid (will add it to exclusion list)
00:09:36.40 +51:34:03.6 -- not an asteroid (will add it to exclusion list)
23:38:10.33 +56:01:45.5 -- not an asteroid (will add it to exclusion list)
23:35:51.01 +58:44:14.3 -- not an asteroid (will add it to exclusion list)
00:25:19.46 +54:00:14.1 -- not an asteroid (will add it to exclusion list)
00:01:06.96 +52:14:04.4 -- not an asteroid (will add it to exclusion list)
00:03:21.40 +55:40:50.9 -- not an asteroid (will add it to exclusion list)
23:43:02.08 +52:58:19.8 -- not an asteroid (will add it to exclusion list)
00:16:54.67 +57:31:48.6 -- not an asteroid (will add it to exclusion list)
00:10:08.98 +54:52:34.5 -- not an asteroid (will add it to exclusion list)
00:09:14.19 +55:08:31.2 -- not an asteroid (will add it to exclusion list)
23:40:53.89 +53:15:41.5 -- not an asteroid (will add it to exclusion list)
23:48:15.12 +56:52:54.4 -- not an asteroid (will add it to exclusion list)
00:05:52.54 +55:02:01.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:51.65 +56:11:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:06.96 +52:14:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:21.40 +55:40:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:04.99 +52:22:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:52.54 +55:02:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:55.85 +53:01:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:14.19 +55:08:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:36.40 +51:34:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:39.51 +53:10:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:08.98 +54:52:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:48.25 +57:29:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:18.29 +53:11:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:50.31 +57:32:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:54.67 +57:31:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:20.40 +51:21:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:19.46 +54:00:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:48.16 +53:16:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:42.32 +48:36:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:33.01 +57:59:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:35.33 +58:18:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:03:47.41 +57:54:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:02.47 +58:13:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:18.86 +58:31:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:39.84 +58:34:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:00.39 +57:39:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:11.38 +56:14:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:05:43.15 +57:00:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:19.18 +57:19:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:21.65 +57:32:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:27.75 +55:38:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:31.34 +55:43:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:36.13 +57:42:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:53.84 +56:42:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:06:57.04 +54:57:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:07.11 +56:00:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:09.31 +58:33:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:37.72 +55:44:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:37.82 +58:37:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:10.63 +58:15:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:16.74 +56:18:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:26.67 +55:49:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:32.28 +53:33:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:32.89 +56:01:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:41.17 +58:18:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:42.25 +55:33:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:43.94 +55:52:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:52.06 +57:47:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:19.54 +54:58:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:21.89 +55:50:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:25.64 +53:47:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:27.13 +55:23:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:59.02 +53:37:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:02.71 +58:41:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:30.86 +58:26:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:52.61 +50:48:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:55.86 +53:27:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:30.90 +50:56:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:38.84 +58:43:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:40.79 +56:27:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:44.96 +51:11:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:52.99 +53:32:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:00.25 +51:10:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:00.28 +54:37:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:04.20 +54:28:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:15.28 +55:01:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:19.26 +53:42:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:22.31 +52:05:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:25.34 +53:51:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:27.51 +53:25:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:29.99 +50:52:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:38.78 +53:54:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:15.27 +52:46:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:28.54 +55:16:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:29.74 +53:42:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:30.61 +54:23:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:33.98 +53:34:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:38.06 +56:48:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:43.83 +53:17:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:10.23 +52:32:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:14.19 +49:05:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:28.64 +52:51:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:29.46 +51:30:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:32.26 +53:17:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:56.39 +55:55:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:11.49 +53:51:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:16.53 +55:01:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:33.51 +58:28:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:50.84 +52:57:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:58.43 +52:22:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:00.21 +50:50:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:03.91 +52:59:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:26.88 +58:49:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:28.99 +53:45:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:31.99 +55:54:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:40.54 +56:43:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:48.90 +54:33:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:51.50 +51:00:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:05.82 +55:40:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:07.49 +54:06:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:09.24 +52:58:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:09.27 +58:40:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:33.86 +54:23:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:45.44 +51:22:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:47.71 +53:46:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:50.93 +55:58:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.94 +56:15:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:32.10 +56:13:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:32.11 +49:23:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:41.13 +53:03:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:53.05 +56:57:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:02.84 +49:36:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:10.60 +58:47:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:24.77 +55:31:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:44.78 +57:52:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:09.78 +49:01:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:17.63 +56:04:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:27.78 +58:22:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:30.88 +57:53:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:43.73 +50:16:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:03.16 +58:13:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:12.29 +49:05:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:44.87 +48:59:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:12.12 +49:02:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:13.06 +57:09:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:31.53 +49:00:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:32.54 +57:39:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:34.51 +49:16:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:03.02 +57:21:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:26.64 +50:09:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:05.09 +58:25:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:18.02 +56:06:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:47.41 +56:18:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:54.43 +49:05:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:12.57 +54:32:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:29.17 +58:01:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:31.38 +49:29:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:51.31 +50:08:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:35.59 +55:43:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:22.33 +49:35:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:56.01 +57:57:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:47.18 +58:29:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:05.03 +55:03:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:07.22 +49:12:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:50.68 +58:46:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:18.60 +49:25:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:47.54 +53:41:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:48.15 +58:51:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:51.01 +58:44:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:09.46 +58:47:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:38.97 +53:07:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:40.16 +58:50:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:10.33 +56:01:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:57.42 +56:10:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:53.89 +53:15:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:02.08 +52:58:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:12.33 +57:41:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:32.33 +56:34:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:11.25 +56:01:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:12.80 +58:54:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:15.12 +56:52:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:56.51 +54:48:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:54.77 +53:12:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:23.12 +53:19:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:48.42 +53:24:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:58.44 +56:44:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:41.17 +56:24:11.1 -- 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)
00:00:51.65 +56:11:55.1 -- a known variable star
00:01:06.96 +52:14:04.4 -- a known variable star
00:03:21.40 +55:40:50.9 -- a known variable star
00:05:04.99 +52:22:05.5 -- not a known variable star
00:05:52.54 +55:02:01.6 -- a known variable star
00:07:55.85 +53:01:06.0 -- a known variable star
00:09:14.19 +55:08:31.2 -- a known variable star
00:09:36.40 +51:34:03.6 -- a known variable star
00:09:39.51 +53:10:14.8 -- a known variable star
00:10:08.98 +54:52:34.5 -- a known variable star
00:10:48.25 +57:29:23.4 -- a known variable star
00:15:18.29 +53:11:56.7 -- a known variable star
00:15:50.31 +57:32:36.7 -- a known variable star
00:16:54.67 +57:31:48.6 -- a known variable star
00:21:20.40 +51:21:41.6 -- a known variable star
00:25:19.46 +54:00:14.1 -- a known variable star
00:29:48.16 +53:16:48.6 -- not a known variable star
00:44:42.32 +48:36:30.5 -- a known variable star
23:03:33.01 +57:59:54.1 -- not a known variable star
23:03:35.33 +58:18:40.4 -- a known variable star
23:03:47.41 +57:54:28.8 -- not a known variable star
23:04:02.47 +58:13:01.6 -- a known variable star
23:04:18.86 +58:31:23.9 -- a known variable star
23:04:39.84 +58:34:38.4 -- a known variable star
23:05:00.39 +57:39:10.5 -- a known variable star
23:05:11.38 +56:14:55.1 -- not a known variable star
23:05:43.15 +57:00:23.8 -- not a known variable star
23:06:19.18 +57:19:32.8 -- not a known variable star
23:06:21.65 +57:32:45.6 -- not a known variable star
23:06:27.75 +55:38:39.4 -- not a known variable star
23:06:31.34 +55:43:26.8 -- not a known variable star
23:06:36.13 +57:42:22.9 -- not a known variable star
23:06:53.84 +56:42:52.0 -- not a known variable star
23:06:57.04 +54:57:57.2 -- a known variable star
23:07:07.11 +56:00:24.8 -- a known variable star
23:07:09.31 +58:33:17.4 -- a known variable star
23:07:37.72 +55:44:19.8 -- not a known variable star
23:07:37.82 +58:37:21.9 -- not a known variable star
23:08:10.63 +58:15:54.3 -- not a known variable star
23:08:16.74 +56:18:24.7 -- a known variable star
23:08:26.67 +55:49:47.7 -- not a known variable star
23:08:32.28 +53:33:12.4 -- not a known variable star
23:08:32.89 +56:01:01.2 -- not a known variable star
23:08:41.17 +58:18:06.9 -- a known variable star
23:08:42.25 +55:33:08.2 -- a known variable star
23:08:43.94 +55:52:27.8 -- a known variable star
23:08:52.06 +57:47:52.1 -- not a known variable star
23:09:19.54 +54:58:17.4 -- a known variable star
23:09:21.89 +55:50:10.1 -- not a known variable star
23:09:25.64 +53:47:19.3 -- not a known variable star
23:09:27.13 +55:23:03.3 -- not a known variable star
23:09:59.02 +53:37:49.1 -- not a known variable star
23:10:02.71 +58:41:25.2 -- not a known variable star
23:10:30.86 +58:26:14.0 -- not a known variable star
23:10:52.61 +50:48:05.3 -- not a known variable star
23:10:55.86 +53:27:56.6 -- a known variable star
23:11:30.90 +50:56:33.5 -- not a known variable star
23:11:38.84 +58:43:39.5 -- not a known variable star
23:11:40.79 +56:27:41.9 -- not a known variable star
23:11:44.96 +51:11:15.3 -- not a known variable star
23:11:52.99 +53:32:26.3 -- a known variable star
23:12:00.25 +51:10:32.8 -- a known variable star
23:12:00.28 +54:37:16.0 -- a known variable star
23:12:04.20 +54:28:23.8 -- a known variable star
23:12:15.28 +55:01:59.5 -- not a known variable star
23:12:19.26 +53:42:43.8 -- a known variable star
23:12:22.31 +52:05:19.2 -- not a known variable star
23:12:25.34 +53:51:03.9 -- not a known variable star
23:12:27.51 +53:25:44.3 -- not a known variable star
23:12:29.99 +50:52:36.3 -- not a known variable star
23:12:38.78 +53:54:03.1 -- not a known variable star
23:13:15.27 +52:46:41.3 -- a known variable star
23:13:28.54 +55:16:55.7 -- not a known variable star
23:13:29.74 +53:42:18.1 -- a known variable star
23:13:30.61 +54:23:54.0 -- a known variable star
23:13:33.98 +53:34:16.3 -- not a known variable star
23:13:38.06 +56:48:20.0 -- not a known variable star
23:13:43.83 +53:17:38.1 -- not a known variable star
23:14:10.23 +52:32:51.6 -- not a known variable star
23:14:14.19 +49:05:42.7 -- a known variable star
23:14:28.64 +52:51:44.6 -- not a known variable star
23:14:29.46 +51:30:48.1 -- not a known variable star
23:14:32.26 +53:17:07.5 -- not a known variable star
23:14:56.39 +55:55:22.1 -- not a known variable star
23:15:11.49 +53:51:44.7 -- a known variable star
23:15:16.53 +55:01:21.9 -- a known variable star
23:15:33.51 +58:28:46.6 -- not a known variable star
23:15:50.84 +52:57:36.9 -- not a known variable star
23:15:58.43 +52:22:28.7 -- not a known variable star
23:16:00.21 +50:50:51.8 -- a known variable star
23:16:03.91 +52:59:24.8 -- not a known variable star
23:16:26.88 +58:49:08.5 -- not a known variable star
23:16:28.99 +53:45:30.8 -- not a known variable star
23:16:31.99 +55:54:09.8 -- not a known variable star
23:16:40.54 +56:43:17.9 -- not a known variable star
23:16:48.90 +54:33:26.6 -- not a known variable star
23:16:51.50 +51:00:45.1 -- a known variable star
23:17:05.82 +55:40:24.9 -- a known variable star
23:18:07.49 +54:06:43.0 -- not a known variable star
23:18:09.24 +52:58:29.7 -- not a known variable star
23:18:09.27 +58:40:45.9 -- not a known variable star
23:18:33.86 +54:23:59.2 -- a known variable star
23:18:45.44 +51:22:46.1 -- not a known variable star
23:18:47.71 +53:46:04.8 -- a known variable star
23:18:50.93 +55:58:43.7 -- not a known variable star
23:18:56.94 +56:15:28.5 -- not a known variable star
23:19:32.10 +56:13:42.5 -- a known variable star
23:19:32.11 +49:23:44.2 -- not a known variable star
23:19:41.13 +53:03:08.3 -- not a known variable star
23:19:53.05 +56:57:33.3 -- a known variable star
23:20:02.84 +49:36:34.6 -- not a known variable star
23:20:10.60 +58:47:09.3 -- not a known variable star
23:20:24.77 +55:31:27.0 -- a known variable star
23:20:44.78 +57:52:27.7 -- not a known variable star
23:21:09.78 +49:01:55.5 -- not a known variable star
23:21:17.63 +56:04:44.1 -- a known variable star
23:21:27.78 +58:22:08.2 -- not a known variable star
23:21:30.88 +57:53:52.7 -- not a known variable star
23:21:43.73 +50:16:58.3 -- not a known variable star
23:22:03.16 +58:13:01.6 -- a known variable star
23:22:12.29 +49:05:33.2 -- not a known variable star
23:22:44.87 +48:59:09.0 -- not a known variable star
23:23:12.12 +49:02:28.4 -- a known variable star
23:23:13.06 +57:09:34.0 -- not a known variable star
23:23:31.53 +49:00:05.7 -- not a known variable star
23:23:32.54 +57:39:03.3 -- not a known variable star
23:23:34.51 +49:16:56.8 -- not a known variable star
23:24:03.02 +57:21:01.3 -- not a known variable star
23:24:26.64 +50:09:59.2 -- not a known variable star
23:25:05.09 +58:25:07.5 -- not a known variable star
23:25:18.02 +56:06:27.5 -- a known variable star
23:25:47.41 +56:18:54.2 -- a known variable star
23:25:54.43 +49:05:43.4 -- not a known variable star
23:26:12.57 +54:32:12.5 -- a known variable star
23:26:29.17 +58:01:45.9 -- not a known variable star
23:26:31.38 +49:29:39.6 -- a known variable star
23:26:51.31 +50:08:05.1 -- not a known variable star
23:27:35.59 +55:43:18.0 -- a known variable star
23:28:22.33 +49:35:07.3 -- not a known variable star
23:28:56.01 +57:57:15.8 -- not a known variable star
23:29:47.18 +58:29:35.6 -- not a known variable star
23:30:05.03 +55:03:39.8 -- not a known variable star
23:30:07.22 +49:12:19.0 -- not a known variable star
23:31:50.68 +58:46:18.2 -- not a known variable star
23:33:18.60 +49:25:54.1 -- not a known variable star
23:33:47.54 +53:41:03.9 -- a known variable star
23:34:48.15 +58:51:33.3 -- not a known variable star
23:35:51.01 +58:44:14.3 -- a known variable star
23:36:09.46 +58:47:01.4 -- not a known variable star
23:37:38.97 +53:07:18.8 -- a known variable star
23:37:40.16 +58:50:41.5 -- a known variable star
23:38:10.33 +56:01:45.5 -- a known variable star
23:39:57.42 +56:10:19.5 -- a known variable star
23:40:53.89 +53:15:41.5 -- a known variable star
23:43:02.08 +52:58:19.8 -- a known variable star
23:43:12.33 +57:41:43.0 -- not a known variable star
23:44:32.33 +56:34:50.2 -- a known variable star
23:47:11.25 +56:01:23.7 -- not a known variable star
23:47:12.80 +58:54:07.1 -- a known variable star
23:48:15.12 +56:52:54.4 -- a known variable star
23:51:56.51 +54:48:08.2 -- a known variable star
23:53:54.77 +53:12:53.4 -- a known variable star
23:54:23.12 +53:19:24.0 -- a known variable star
23:56:48.42 +53:24:18.7 -- a known variable star
23:56:58.44 +56:44:52.7 -- a known variable star
23:59:41.17 +56:24:11.1 -- a known variable star
Found 92 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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166 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)2461093.59754242 -observatory 500
23:23:17.46 -02:00:57.1 Mercury (-0.1mag)
23:04:08.31 -07:31:53.5 Venus (-3.9mag)
21:42:35.73 -14:53:55.7 Mars (1.1mag)
07:06:07.02 +22:54:18.1 Jupiter (-2.5mag)
00:05:24.40 -01:44:39.9 Saturn (1.0mag)
03:39:59.22 +19:21:42.7 Uranus (5.7mag)
00:03:40.36 -01:01:40.9 Neptune (7.8mag)
20:29:06.53 -22:59:35.4 Pluto (14.5mag)
01:50:29.87 +15:51:27.5 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Feb 21 20:31 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.59754242:
07:06:09.42 +22:54:16.2 Io (5.4mag)
07:06:17.68 +22:53:59.0 Europa (5.5mag)
07:05:56.65 +22:54:45.7 Ganymede (4.9mag)
07:06:25.24 +22:53:54.3 Callisto (6.2mag)
07:09:15.70 +23:10:42.9 Himalia (15.0mag)
07:06:05.92 +22:54:22.5 Thebe (15.9mag)
07:08:40.83 +23:19:09.2 Elara (17.0mag)
07:01:40.37 +24:02:18.4 Pasiphae (17.0mag)
07:15:07.92 +22:42:17.0 Carme (18.1mag)
00:05:36.03 -01:44:44.7 Titan (8.8mag)
00:05:29.72 -01:44:38.7 Rhea (10.1mag)
00:05:19.64 -01:46:01.2 Iapetus (11.5mag)
00:05:25.01 -01:44:42.8 Hyperion (14.8mag)
00:07:28.69 -01:31:39.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 21 20:31 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.59754242:
08:45:20.43 +24:30:39.3 JWST
10:06:06.21 +36:18:21.7 Chandra
14:40:55.69 -62:29:57.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 21 20:31 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)2461093.59754242 at 500
16:59:35.01 -11:03:46.6 17.5mag 10P/Tempel 2
03:37:15.45 +28:57:37.5 18.0mag 123P/West-Hartley
08:23:44.14 +60:43:56.2 18.4mag 124P/Mrkos
21:19:23.29 -07:39:44.1 22.1mag 141P/Machholz
01:21:01.37 +11:53:53.1 17.6mag 145P/Shoemaker-Levy 5
11:03:02.28 +30:34:09.2 17.9mag 164P/Christensen
09:33:09.86 -33:51:57.0 18.0mag 195P/Hill
15:52:03.59 -06:36:12.6 19.2mag 210P/Christensen
18:16:35.56 -21:28:42.6 17.3mag 218P/LINEAR
16:21:28.35 -18:11:01.2 15.2mag 235P/LINEAR
03:56:18.48 +27:43:53.2 17.8mag 240P/NEAT
15:17:33.76 +06:38:40.4 14.8mag 24P/Schaumasse
11:23:32.46 -03:23:14.9 17.4mag 29P/Schwassmann-Wachmann 1
07:03:48.29 +27:24:48.8 19.6mag 407P/PanSTARRS-Fuls
17:07:03.09 -11:19:15.8 17.6mag 40P/Vaisala 1
11:02:15.08 -08:52:04.4 16.6mag 43P/Wolf-Harrington
13:25:29.53 -05:49:28.3 20.0mag 489P/Denning
04:34:19.56 +48:34:50.6 17.8mag 493P/2024 Q2 (LONEOS)
06:04:21.84 +47:32:05.4 17.7mag 63P/Wild 1
23:14:29.76 -02:08:08.3 16.2mag 78P/Gehrels 2
20:01:17.57 -22:18:47.7 15.0mag 88P/Howell
15:27:52.98 -29:00:24.7 18.7mag P/2023 S1 (PanSTARRS)
04:43:26.79 -72:36:06.0 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.48 +31:12:53.6 18.2mag C/2017 K2 (PanSTARRS)
20:06:36.38 -65:11:31.9 18.1mag C/2020 V2 (ZTF)
17:21:38.99 +04:21:01.9 16.3mag C/2021 G2 (ATLAS)
03:35:38.32 +24:36:38.2 15.8mag C/2022 N2 (PanSTARRS)
09:08:14.41 +29:49:18.2 15.3mag C/2022 QE78 (ATLAS)
08:35:41.57 -06:34:11.6 16.7mag C/2022 R6 (PanSTARRS)
23:52:57.96 +48:26:37.3 18.0mag C/2023 C2 (ATLAS)
09:51:11.51 -20:46:28.3 17.5mag C/2023 F3 (ATLAS)
20:34:38.61 +61:14:30.7 17.3mag C/2023 H5 (Lemmon)
19:34:29.74 -03:24:14.3 16.1mag C/2023 R1 (PANSTARRS)
02:48:54.16 +35:40:35.8 18.5mag C/2023 RS61 (PanSTARRS)
21:01:21.50 +81:19:52.3 18.0mag C/2023 X2 (Lemmon)
06:39:14.59 +63:49:08.8 17.3mag C/2024 A1 (ATLAS)
01:56:20.91 -24:42:22.4 11.2mag C/2024 E1 (Wierzchos)
11:45:01.30 -02:35:28.5 18.1mag C/2024 G2 (ATLAS)
19:28:15.82 +00:39:05.9 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.83 -01:43:18.6 17.7mag C/2024 G6 (ATLAS)
19:53:25.32 +03:14:30.6 15.6mag C/2024 J3 (ATLAS)
02:47:12.85 -31:35:06.2 15.4mag C/2024 T5 (ATLAS)
16:25:15.01 -58:12:32.3 15.6mag C/2025 A6 (Lemmon)
04:50:30.14 +62:15:48.8 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:45.71 -13:03:59.6 14.8mag C/2025 L1 (ATLAS)
02:20:11.28 -19:05:30.5 16.7mag C/2025 Q3 (ATLAS)
02:09:30.32 +17:16:25.3 21.2mag C/2025 R2 (SWAN)
22:20:44.68 +17:39:10.0 16.4mag C/2025 R3 (PANSTARRS)
21:45:57.77 -16:49:43.4 21.5mag C/2025 T1 (ATLAS)
03:06:21.93 -20:35:37.0 18.3mag C/2026 A1 (MAPS)
21:02:49.71 +20:54:09.1 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 21 20:31 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
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############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 21 20:31 tocp_transients_list.txt