This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9
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 22.2714 2461093.7714 10.37 07:33:26.27 +57:47:50.2
159.40639 28.18181 galactic Lyn Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J113.3486+57.8020 | 07:33:27.12 +57:47:52.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J113.3486+57.8020,2461093.7714,10.37,0.05,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 J113.3486+57.8020 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:26.27 +57:47:50.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0804359+562135,2461093.7714,11.09,0.05,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
NSVS J0804359+562135 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:35.78 +56:21:35.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.93 08:02:45.70 +52:44:30.0
165.66570 31.86447 galactic Lyn Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:02:45.70 +52:44:30.0 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.051 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.93,0.05,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
target 20260222.2714 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:02:45.70 +52:44:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.74 08:00:48.23 +54:07:56.4
164.01109 31.66457 galactic Lyn Second-epoch detections are separated by 3.9" 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 | target | 08:00:48.23 +54:07:56.4 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.74,0.05,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
target 20260222.2714 13.74CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:00:48.23 +54:07:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.90 08:06:41.30 +53:24:12.5
164.92658 32.49253 galactic Lyn Second-epoch detections are separated by 2.6" 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 | target | 08:06:41.30 +53:24:12.5 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.053 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.90,0.05,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
target 20260222.2714 13.90CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:41.30 +53:24:12.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.51 07:37:35.15 +55:38:53.4
161.90882 28.48276 galactic Lyn Second-epoch detections are separated by 5.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:37:35.15 +55:38:53.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:35.15 +55:38:53.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.78 08:24:02.85 +58:57:22.6
158.21641 34.82892 galactic Lyn Second-epoch detections are separated by 1.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:24:02.85 +58:57:22.6 (user input) | T | P | (position from user input) J-Ks=0.400+/- (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.78CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:02.85 +58:57:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:02.08 +57:52:50.9 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.56 08:06:08.26 +49:02:14.8
170.06995 32.08314 galactic Lyn Second-epoch detections are separated by 2.5" 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 | target | 08:06:08.26 +49:02:14.8 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:08.26 +49:02:14.8 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.70 08:29:05.31 +55:04:05.3
162.91646 35.76449 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:29:05.31 +55:04:05.3 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.065 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.70,0.05,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
target 20260222.2714 13.70CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:05.31 +55:04:05.3 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.88,0.05,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
target 20260222.2714 13.88CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:20.06 +57:39:30.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.38 08:04:31.04 +51:21:15.9
167.31970 32.03067 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J121.1343+51.3564 | 08:04:31.04 +51:21:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.340+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J121.1343+51.3564,2461093.7714,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J121.1343+51.3564 20260222.2714 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:31.04 +51:21:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.31 07:35:54.59 +56:58:53.8
160.37130 28.41507 galactic Lyn Second-epoch detections are separated by 2.2" 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 | target | 07:35:54.59 +56:58:53.8 (user input) | T | P | (position from user input) 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:54.59 +56:58:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.36 07:39:49.02 +58:29:22.2
158.72324 29.09180 galactic Lyn Second-epoch detections are separated by 3.9" 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 J114.9602+58.5011 | 07:39:49.02 +58:29:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J114.9602+58.5011,2461093.7714,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J114.9602+58.5011 20260222.2714 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:49.02 +58:29:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:21.68 +58:41:28.8 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.39 08:16:03.36 +58:22:27.0
158.99551 33.82682 galactic Lyn Second-epoch detections are separated by 0.9" 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 | target | 08:16:03.36 +58:22:27.0 (user input) | T | P | (position from user input) J-Ks=0.608+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:03.36 +58:22:27.0 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.35 07:35:45.61 +58:16:49.4
158.90063 28.54205 galactic Lyn Second-epoch detections are separated by 4.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:35:45.61 +58:16:49.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.35,0.05,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
target 20260222.2714 13.35CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:45.61 +58:16:49.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:54.68 +57:19:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.16 08:07:56.59 +55:02:27.2
162.99222 32.73774 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:07:56.59 +55:02:27.2 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:56.59 +55:02:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:11.36 +58:27:05.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:33.22 +57:53:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.01 07:35:17.46 +58:24:10.8
158.75436 28.49403 galactic Lyn Second-epoch detections are separated by 4.8" 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 | target | 07:35:17.46 +58:24:10.8 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:17.46 +58:24:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.04 07:34:57.58 +56:29:31.9
160.90488 28.22566 galactic Lyn Second-epoch detections are separated by 2.3" 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 | target | 07:34:57.58 +56:29:31.9 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:57.58 +56:29:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:47.10 +56:47:51.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.82 07:49:58.73 +51:44:41.7
166.60253 29.82133 galactic Lyn Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:49:58.73 +51:44:41.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.521+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:49:58.73 +51:44:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.72 07:35:30.82 +57:28:50.8
159.80052 28.42037 galactic Lyn Second-epoch detections are separated by 1.1" 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 | ATO J113.8818+57.4814 | 07:35:31.65 +57:28:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J113.8818+57.4814,2461093.7714,12.72,0.05,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 J113.8818+57.4814 20260222.2714 12.72CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:30.82 +57:28:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.04 07:33:30.92 +56:35:02.6
160.77250 28.04006 galactic Lyn Second-epoch detections are separated by 2.8" 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 | ATO J113.3731+56.5801 | 07:33:29.65 +56:35:03.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J113.3731+56.5801,2461093.7714,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J113.3731+56.5801 20260222.2714 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:30.92 +56:35:02.6 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.02 07:33:35.43 +55:55:45.6
161.50896 27.96286 galactic Lyn Second-epoch detections are separated by 2.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 989104167673502336 | 07:33:33.85 +55:55:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989104167673502336,2461093.7714,12.02,0.05,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 989104167673502336 20260222.2714 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:35.43 +55:55:45.6 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.90 07:32:48.15 +56:59:29.8
160.30037 27.99635 galactic Lyn Second-epoch detections are separated by 1.1" 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 989220239165083136 | 07:32:46.97 +56:59:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989220239165083136,2461093.7714,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 989220239165083136 20260222.2714 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:48.15 +56:59:29.8 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.97 08:03:46.18 +57:19:10.9
160.27708 32.20563 galactic Lyn Second-epoch detections are separated by 1.3" 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 | target | 08:03:46.18 +57:19:10.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.370+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:46.18 +57:19:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.84 07:37:56.32 +58:12:07.0
159.02346 28.81902 galactic Lyn Second-epoch detections are separated by 2.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1085424306843848960 | 07:37:57.28 +58:12:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1085424306843848960,2461093.7714,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1085424306843848960 20260222.2714 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:56.32 +58:12:07.0 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.67 07:34:42.45 +56:39:57.9
160.70414 28.21319 galactic Lyn Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 989152511824785920 | 07:34:41.25 +56:39:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989152511824785920,2461093.7714,11.67,0.05,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
Gaia DR3 989152511824785920 20260222.2714 11.67CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:42.45 +56:39:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.43 07:36:18.42 +57:09:53.8
160.17143 28.49018 galactic Lyn Second-epoch detections are separated by 2.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 989283632882830336 | 07:36:19.35 +57:09:55.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989283632882830336,2461093.7714,11.43,0.05,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 989283632882830336 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:18.42 +57:09:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a 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 22.2714* 09 10 28.33 +52 41 21.2 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1022632748266050688,2461093.7714,10.60,0.05,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 1022632748266050688 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:28.33 +52:41:21.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 10.03 07:40:34.93 +58:26:28.0
158.78869 29.18711 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1085518353744505856 | 07:40:35.98 +58:26:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1085518353744505856,2461093.7714,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1085518353744505856 20260222.2714 10.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:40:34.93 +58:26:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.05 08:14:03.24 +49:24:37.9
169.75763 33.40251 galactic Lyn Second-epoch detections are separated by 0.9" 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 931663829108723712 | 08:14:05.32 +49:24:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 931663829108723712,2461093.7714,11.05,0.05,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 931663829108723712 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:03.24 +49:24:37.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 11.63 07:34:19.47 +58:09:21.4
159.01755 28.34043 galactic Lyn Second-epoch detections are separated by 3.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1085452451766164096 | 07:34:20.22 +58:09:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1085452451766164096,2461093.7714,11.63,0.05,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
Gaia DR3 1085452451766164096 20260222.2714 11.63CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:19.47 +58:09:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.05 07:56:16.97 +53:45:57.2
164.38369 30.97509 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J119.0817+53.7680 | 07:56:16.97 +53:45:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.355+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J119.0817+53.7680,2461093.7714,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J119.0817+53.7680 20260222.2714 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:56:16.97 +53:45:57.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.26 07:31:05.44 +58:13:05.1
158.89009 27.92468 galactic Lyn Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 989576412213950720 | 07:31:06.28 +58:13:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989576412213950720,2461093.7714,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 989576412213950720 20260222.2714 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:05.44 +58:13:05.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.46 07:36:01.52 +56:32:38.1
160.86740 28.37794 galactic Lyn Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 986146790631801344 | 07:35:57.45 +56:32:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 986146790631801344,2461093.7714,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 986146790631801344 20260222.2714 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:01.52 +56:32:38.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.52 07:58:44.51 +57:15:32.9
160.32784 31.52506 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1081741634381588992 | 07:58:47.18 +57:15:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.193+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1081741634381588992,2461093.7714,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1081741634381588992 20260222.2714 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:58:44.51 +57:15:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.80 07:31:51.09 +57:58:09.5
159.18370 27.99353 galactic Lyn Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 989381450762454528 | 07:31:51.81 +57:58:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 989381450762454528,2461093.7714,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 989381450762454528 20260222.2714 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:51.09 +57:58:09.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1085459907829407360,2461093.7714,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1085459907829407360 20260222.2714 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:49.55 +58:06:03.7 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.96 08:15:07.93 +55:00:04.7
163.05674 33.76738 galactic Lyn Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1033067182332467072 | 08:15:03.26 +55:00:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1033067182332467072,2461093.7714,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1033067182332467072 20260222.2714 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:07.93 +55:00:04.7 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:11.73 +58:05:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.04 08:11:50.52 +49:33:53.3
169.54256 33.05540 galactic Lyn Second-epoch detections are separated by 0.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:11:50.52 +49:33:53.3 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:50.52 +49:33:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.19 07:33:03.73 +57:22:33.4
159.87356 28.08020 galactic Lyn Second-epoch detections are separated by 3.1" 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 | target | 07:33:03.73 +57:22:33.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:03.73 +57:22:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:04.51 +58:01:16.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.16 07:58:10.51 +51:12:03.6
167.39427 31.02908 galactic Lyn Second-epoch detections are separated by 2.1" 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 | target | 07:58:10.51 +51:12:03.6 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.043 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:58:10.51 +51:12:03.6 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.25 08:18:50.04 +56:16:22.1
161.51477 34.27349 galactic Lyn Second-epoch detections are separated by 0.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J124.7082+56.2716 | 08:18:50.04 +56:16:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J124.7082+56.2716,2461093.7714,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J124.7082+56.2716 20260222.2714 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:18:50.04 +56:16:22.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.30 08:17:21.05 +52:15:09.2
166.37416 34.05884 galactic Lyn Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:17:21.05 +52:15:09.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.606+/-0.040 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:21.05 +52:15:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0816245+492913,2461093.7714,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0816245+492913 20260222.2714 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:24.41 +49:29:13.6 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.54 08:29:48.66 +56:04:33.4
161.66890 35.80847 galactic Lyn Second-epoch detections are separated by 0.7" 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 1033819351365122944 | 08:29:51.91 +56:05:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.440+/-0.055 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1033819351365122944,2461093.7714,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1033819351365122944 20260222.2714 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:48.66 +56:04:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.7714,13.42,0.05,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
VARIABLE_NAME 20260222.2714 13.42CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:50.11 +48:55:55.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.62 07:34:44.72 +57:52:57.3
159.33337 28.36461 galactic Lyn Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:34:44.72 +57:52:57.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:44.72 +57:52:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.48 08:17:54.11 +50:08:08.5
168.93161 34.06577 galactic Lyn Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:17:54.11 +50:08:08.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.48,0.05,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
target 20260222.2714 13.48CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:54.11 +50:08:08.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.65 08:59:43.33 +58:30:39.8
157.91757 39.46962 galactic UMa Second-epoch detections are separated by 0.6" 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 1037642731252764160 | 08:59:39.21 +58:31:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 59 43.33 +58 30 39.8 13.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1037642731252764160,2461093.7714,13.65,0.05,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 1037642731252764160 20260222.2714 13.65CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:43.33 +58:30:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a 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 22.2714* 08 45 23.06 +55 11 44.6 13.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LINEAR 5148766,2461093.7714,13.59,0.05,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
LINEAR 5148766 20260222.2714 13.59CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:45:23.06 +55:11:44.6 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.63,0.05,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
target 20260222.2714 13.63CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:44.80 +58:28:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.62 08:07:33.55 +49:02:17.8
170.09557 32.31510 galactic Lyn Second-epoch detections are separated by 1.0" 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 934604163718517760 | 08:07:30.77 +49:02:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.339+/-0.044 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 934604163718517760,2461093.7714,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 934604163718517760 20260222.2714 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:33.55 +49:02:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.60 07:52:49.62 +50:19:49.1
168.28684 30.08968 galactic Lyn Second-epoch detections are separated by 1.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:52:49.62 +50:19:49.1 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.60,0.05,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
target 20260222.2714 13.60CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:49.62 +50:19:49.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.55 08:30:37.64 +51:06:21.3
167.80074 36.10491 galactic Lyn Second-epoch detections are separated by 3.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1028129413051719936 | 08:30:34.20 +51:05:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1028129413051719936,2461093.7714,13.55,0.05,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 1028129413051719936 20260222.2714 13.55CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:37.64 +51:06:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.89 08:38:01.66 +52:01:21.1
166.62404 37.23270 galactic UMa Second-epoch detections are separated by 1.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:38:01.66 +52:01:21.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.355+/-0.055 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 38 01.66 +52 01 21.1 13.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.89,0.05,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
target 20260222.2714 13.89CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:38:01.66 +52:01:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.93 08:02:58.18 +53:38:06.6
164.61770 31.95316 galactic Lyn Second-epoch detections are separated by 1.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:02:58.18 +53:38:06.6 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.066 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.93,0.05,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
target 20260222.2714 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:02:58.18 +53:38:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.82 08:13:01.44 +54:31:15.9
163.63046 33.45948 galactic Lyn Second-epoch detections are separated by 2.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:13:01.44 +54:31:15.9 (user input) | T | P | (position from user input) J-Ks=0.984+/-0.111 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:01.44 +54:31:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.77 08:19:18.12 +55:55:20.4
161.93690 34.34775 galactic Lyn Second-epoch detections are separated by 1.3" 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 | target | 08:19:18.12 +55:55:20.4 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.061 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.77,0.05,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
target 20260222.2714 13.77CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:19:18.12 +55:55:20.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.92 08:21:42.68 +50:00:19.9
169.12144 34.67078 galactic Lyn Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:21:42.68 +50:00:19.9 (user input) | T | P | (position from user input) J-Ks=0.582+/-0.051 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.92,0.05,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
target 20260222.2714 13.92CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:42.68 +50:00:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.84 08:09:55.59 +55:33:44.5
162.37811 33.03039 galactic Lyn Second-epoch detections are separated by 1.7" 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 | target | 08:09:55.59 +55:33:44.5 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.053 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.84,0.05,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
target 20260222.2714 13.84CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:55.59 +55:33:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.79 08:17:42.83 +52:04:08.2
166.59755 34.10965 galactic Lyn Second-epoch detections are separated by 0.1" 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 | target | 08:17:42.83 +52:04:08.2 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.064 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:42.83 +52:04:08.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.87 08:11:54.46 +53:41:57.4
164.61012 33.27853 galactic Lyn Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:11:54.46 +53:41:57.4 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.066 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:54.46 +53:41:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.99 08:20:13.67 +51:04:59.7
167.80359 34.47202 galactic Lyn Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:20:13.67 +51:04:59.7 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.039 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:20:13.67 +51:04:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a 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 22.2714* 08 44 32.92 +55 38 03.2 13.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1030895165832279168,2461093.7714,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1030895165832279168 20260222.2714 13.86CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:44:32.92 +55:38:03.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.97 08:17:46.23 +55:14:16.0
162.76952 34.14346 galactic Lyn Second-epoch detections are separated by 2.4" 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 | target | 08:17:46.23 +55:14:16.0 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.060 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.97,0.05,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
target 20260222.2714 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:46.23 +55:14:16.0 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.96 08:26:40.76 +52:16:14.3
166.36919 35.48628 galactic Lyn Second-epoch detections are separated by 2.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J126.6834+52.2735 | 08:26:40.76 +52:16:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.524+/-0.047 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J126.6834+52.2735,2461093.7714,13.96,0.05,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
ATO J126.6834+52.2735 20260222.2714 13.96CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:40.76 +52:16:14.3 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.86 08:43:33.11 +56:05:22.5
161.43376 37.71587 galactic UMa Second-epoch detections are separated by 0.6" 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 | target | 08:43:33.11 +56:05:22.5 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.053 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 43 33.11 +56 05 22.5 13.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.86,0.05,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
target 20260222.2714 13.86CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:43:33.11 +56:05:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.88 08:16:45.76 +51:28:12.0
167.31419 33.94341 galactic Lyn Second-epoch detections are separated by 0.9" 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 | target | 08:16:45.76 +51:28:12.0 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.052 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.88,0.05,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
target 20260222.2714 13.88CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:45.76 +51:28:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.88 08:32:27.42 +54:28:06.5
163.62549 36.28097 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:32:27.42 +54:28:06.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.524+/-0.051 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.88,0.05,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
target 20260222.2714 13.88CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:32:27.42 +54:28:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.00 08:06:33.81 +54:30:34.0
163.61541 32.52195 galactic Lyn Second-epoch detections are separated by 1.1" 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 | target | 08:06:33.81 +54:30:34.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.485+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.00,0.05,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
target 20260222.2714 14.00CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:33.81 +54:30:34.0 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.06 07:53:14.38 +49:37:44.5
169.10033 30.06450 galactic Lyn Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:53:14.38 +49:37:44.5 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.052 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.06,0.05,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
target 20260222.2714 14.06CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:14.38 +49:37:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.74 08:25:28.73 +52:13:37.8
166.42341 35.30271 galactic Lyn Second-epoch detections are separated by 1.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:25:28.73 +52:13:37.8 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.74,0.05,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
target 20260222.2714 13.74CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:25:28.73 +52:13:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.98 08:08:36.56 +52:36:42.5
165.88253 32.74135 galactic Lyn Second-epoch detections are separated by 2.0" 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 936364756712570368 | 08:08:41.13 +52:36:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.755+/-0.039 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 936364756712570368,2461093.7714,13.98,0.05,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 936364756712570368 20260222.2714 13.98CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:36.56 +52:36:42.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.90 08:16:28.29 +49:57:20.4
169.13382 33.82702 galactic Lyn Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:16:28.29 +49:57:20.4 (user input) | T | P | (position from user input) J-Ks=0.717+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.90,0.05,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
target 20260222.2714 13.90CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:28.29 +49:57:20.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.93 08:48:00.70 +58:37:52.2
158.14002 37.94831 galactic UMa Second-epoch detections are separated by 1.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:48:00.70 +58:37:52.2 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 48 00.70 +58 37 52.2 13.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.93,0.05,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
target 20260222.2714 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:00.70 +58:37:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.12 08:38:40.47 +55:51:14.8
161.81978 37.06245 galactic UMa Second-epoch detections are separated by 1.8" 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 | target | 08:38:40.47 +55:51:14.8 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.061 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 38 40.47 +55 51 14.8 14.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.12,0.05,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
target 20260222.2714 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:38:40.47 +55:51:14.8 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.85 08:12:02.65 +49:06:12.1
170.09450 33.05253 galactic Lyn Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:12:02.65 +49:06:12.1 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:02.65 +49:06:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.95 07:52:01.91 +53:28:17.2
164.65915 30.32095 galactic Lyn Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 984677675594266752 | 07:52:06.01 +53:28:22.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.470+/-0.051 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 984677675594266752,2461093.7714,13.95,0.05,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 984677675594266752 20260222.2714 13.95CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:01.91 +53:28:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.86 08:16:50.27 +49:05:57.4
170.16720 33.83481 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:16:50.27 +49:05:57.4 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.86,0.05,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
target 20260222.2714 13.86CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:50.27 +49:05:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.84 08:55:57.77 +54:37:03.4
163.00717 39.65713 galactic UMa Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1029889520713190272 | 08:55:55.77 +54:36:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.368+/-0.054 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 55 57.77 +54 37 03.4 13.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1029889520713190272,2461093.7714,13.84,0.05,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 1029889520713190272 20260222.2714 13.84CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:57.77 +54:37:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.97 08:07:40.69 +54:24:36.6
163.74008 32.68027 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:07:40.69 +54:24:36.6 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.066 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.97,0.05,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
target 20260222.2714 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:40.69 +54:24:36.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.97 08:33:19.87 +52:03:06.8
166.61871 36.50986 galactic Lyn Second-epoch detections are separated by 0.7" 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 | target | 08:33:19.87 +52:03:06.8 (user input) | T | P | (position from user input) J-Ks=0.777+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.97,0.05,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
target 20260222.2714 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:19.87 +52:03:06.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.80 08:16:47.27 +53:19:27.1
165.07927 33.99579 galactic Lyn Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:16:47.27 +53:19:27.1 (user input) | T | P | (position from user input) J-Ks=0.830+/-0.106 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.80CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:47.27 +53:19:27.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.00 08:23:50.71 +49:51:51.7
169.30819 35.00891 galactic Lyn Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:23:50.71 +49:51:51.7 (user input) | T | P | (position from user input) J-Ks=0.695+/-0.040 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.00,0.05,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
target 20260222.2714 14.00CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:50.71 +49:51:51.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.03 08:04:39.72 +53:03:21.7
165.31761 32.17080 galactic Lyn Second-epoch detections are separated by 1.2" 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 | target | 08:04:39.72 +53:03:21.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.380+/-0.059 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:39.72 +53:03:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.93 08:12:11.82 +52:10:51.4
166.42689 33.26742 galactic Lyn Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:12:11.82 +52:10:51.4 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.049 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.93,0.05,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
target 20260222.2714 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:11.82 +52:10:51.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.96 08:06:32.76 +56:24:07.0
161.37103 32.57014 galactic Lyn Second-epoch detections are separated by 1.8" 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 | target | 08:06:32.76 +56:24:07.0 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.96,0.05,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
target 20260222.2714 13.96CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:32.76 +56:24:07.0 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.09 07:57:42.82 +52:17:01.7
166.12826 31.06209 galactic Lyn Second-epoch detections are separated by 2.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:57:42.82 +52:17:01.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.688+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.09,0.05,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
target 20260222.2714 14.09CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:57:42.82 +52:17:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.84 08:17:41.87 +50:22:47.5
168.63535 34.04490 galactic Lyn Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:17:41.87 +50:22:47.5 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.84,0.05,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
target 20260222.2714 13.84CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:41.87 +50:22:47.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.97 08:22:55.67 +54:34:22.5
163.56180 34.89536 galactic Lyn 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 | target | 08:22:55.67 +54:34:22.5 (user input) | T | P | (position from user input) J-Ks=0.214+/-0.089 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.97,0.05,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
target 20260222.2714 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:22:55.67 +54:34:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.07 08:39:14.67 +57:35:57.3
159.63659 36.95167 galactic UMa Second-epoch detections are separated by 2.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:39:14.67 +57:35:57.3 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.068 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 39 14.67 +57 35 57.3 14.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:39:14.67 +57:35:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.80 08:08:43.10 +55:33:31.6
162.37918 32.85954 galactic Lyn Second-epoch detections are separated by 2.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:08:43.10 +55:33:31.6 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.042 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 13.80CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:43.10 +55:33:31.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.98,0.05,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
target 20260222.2714 13.98CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:52.93 +51:09:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.96,0.05,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
target 20260222.2714 13.96CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:35.55 +51:53:33.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.95 07:51:48.53 +51:58:36.3
166.37518 30.12921 galactic Lyn Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:48.53 +51:58:36.3 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.053 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.95,0.05,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
target 20260222.2714 13.95CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:48.53 +51:58:36.3 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.06 08:26:22.19 +54:32:23.8
163.58538 35.39508 galactic Lyn Second-epoch detections are separated by 1.2" 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 | target | 08:26:22.19 +54:32:23.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.092 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.06,0.05,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
target 20260222.2714 14.06CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:22.19 +54:32:23.8 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.00 08:10:40.42 +51:39:25.9
167.03764 33.00678 galactic Lyn Second-epoch detections are separated by 3.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:10:40.42 +51:39:25.9 (user input) | T | P | (position from user input) J-Ks=0.872+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.00,0.05,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
target 20260222.2714 14.00CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:40.42 +51:39:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 13.77 08:15:26.45 +52:32:07.1
166.02390 33.77535 galactic Lyn Second-epoch detections are separated by 0.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:15:26.45 +52:32:07.1 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.676+/-0.042 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,13.77,0.05,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
target 20260222.2714 13.77CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:26.45 +52:32:07.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.06 08:06:23.34 +53:52:41.1
164.36210 32.47052 galactic Lyn 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 | ATO J121.5978+53.8779 | 08:06:23.34 +53:52:41.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.547+/-0.052 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J121.5978+53.8779,2461093.7714,14.06,0.05,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
ATO J121.5978+53.8779 20260222.2714 14.06CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:23.34 +53:52:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1031702722762235008,2461093.7714,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1031702722762235008 20260222.2714 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:29.64 +52:51:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.05 07:52:58.50 +52:53:05.4
165.35191 30.40330 galactic Lyn Second-epoch detections are separated by 1.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:52:58.50 +52:53:05.4 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.051 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.05,0.05,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
target 20260222.2714 14.05CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:58.50 +52:53:05.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.09 08:07:24.34 +50:18:18.2
168.59911 32.40145 galactic Lyn Second-epoch detections are separated by 0.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:07:24.34 +50:18:18.2 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.397+/-0.076 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.09,0.05,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
target 20260222.2714 14.09CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:24.34 +50:18:18.2 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.03 07:54:25.44 +50:39:49.1
167.94000 30.38263 galactic Lyn Second-epoch detections are separated by 3.8" 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 | target | 07:54:25.44 +50:39:49.1 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:25.44 +50:39:49.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.04 08:40:06.01 +49:52:55.7
169.30492 37.62766 galactic UMa Second-epoch detections are separated by 1.3" 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 | target | 08:40:06.01 +49:52:55.7 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.045 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2714* 08 40 06.01 +49 52 55.7 14.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.04,0.05,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
target 20260222.2714 14.04CV 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:06.01 +49:52:55.7 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 14.13 08:09:20.71 +49:41:15.1
169.35920 32.66191 galactic Lyn Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:09:20.71 +49:41:15.1 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.043 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2714 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:20.71 +49:41:15.1 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2714 2461093.7714 12.44 08:11:21.13 +52:44:23.5
165.75290 33.16256 galactic Lyn Second-epoch detections are separated by 0.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:11:21.13 +52:44:23.5 (user input) | T | P | (position from user input) 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7714,12.44,0.05,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
target 20260222.2714 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:21.13 +52:44:23.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DR Lyn,2461093.7714,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DR Lyn 20260222.2714 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:24.41 +50:00:50.4 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a 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 22.2714* 08 40 49.50 +50 08 14.2 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X UMa,2461093.7714,11.64,0.05,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
X UMa 20260222.2714 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:49.50 +50:08:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20_00sec_-15_00C_LIGHT_0228_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: 2461032.94487828 23.12.2025 10:40:27.483 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
First image: 2461032.94487828 23.12.2025 10:40:27.483 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461093.77166980 22.02.2026 06:31:02.271 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 168
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 8 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): 11706
Objects passed selection criteria: 11696
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 10971.5
Average stars matched: 10485.5 (95.5703 %)
Memory usage VmPeak: 119552 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:26:13 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: 2461032.94487828 23.12.2025 10:40:27.483 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
First image: 2461032.94487828 23.12.2025 10:40:27.483 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461093.77166980 22.02.2026 06:31:02.271 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 318
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 33 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): 62797
Objects passed selection criteria: 62646
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 60104.2
Average stars matched: 57284 (95.3077 %)
Memory usage VmPeak: 165024 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:28:52 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:
Lyn-02-Q2b1x1
#######################################
########### Starting Lyn-02-Q2b1x1 ###########
Processing Lyn-02-Q2b1x1
server tau has sufficient free disk space available: 1042063 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1042063 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.png' -> 'transient_report/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits_preview.png'
Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
renamed 'Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.png' -> 'transient_report/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits_preview.png'
Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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= 478.7291
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 572.9351
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 940.6679
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 594.7497
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 940.4323
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 594.6114
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.96493
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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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: 2461093.77105466
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits'
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:14.834 +54:00:07.16
Angular distance between the image centers 0.08 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 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:13.865 +54:00:35.63
Angular distance between the image centers 0.08 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 08:28:14.834 +54:00:07.16
Second-epoch second image center 08:28:13.865 +54:00:35.63
Angular distance between the image centers 0.00826 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.2G0E0uUWUT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.tqFJECA4UL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.4aAPvF4eCq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.p2jWAQxLKH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits) and catalog (wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat) found
'wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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 22 out of 10919 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.789391
a=0.000000 b=1.000000 c=22.789391
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 166 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
2.1 pix Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
2.4 pix Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
2.4 pix Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
15.4 mag. Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
15.2 mag. Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
15.2 mag. Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.3 (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.2G0E0uUWUT (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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=772, passed=10919
Got 10919 stars (including 10137 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
util/solve_plate_with_UCAC5 got 10919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 164 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: 11.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.40"
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 216 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.19"
Estimated accuracy of the plate solution: 6.84"
Excluding outliers - 190 stars left (next iteration limit 149)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits -region wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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.tqFJECA4UL (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/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=749, passed=10931
Got 10931 stars (including 10170 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
util/solve_plate_with_UCAC5 got 10931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.3'
Seting catalog search parameters based on the expected field of view 927.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012879 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010303 (37.1 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 165 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: 10.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.07"
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 208 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.88"
Estimated accuracy of the plate solution: 7.20"
Excluding outliers - 188 stars left (next iteration limit 147)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits -region wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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.4aAPvF4eCq (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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=907, passed=11112
Got 11112 stars (including 10201 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 11112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.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.p2jWAQxLKH (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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=891, passed=11099
Got 11099 stars (including 10201 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 11099 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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 Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20833.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out20654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20668.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 24s
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: 1s
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Considering the candidate 20637_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20637_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 09:10:28.34 +52:41:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 0.093 1022632748266051072 137.61805452422 +52.68890809952 11.6141 11.0170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20654_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 20654_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 20668_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 20668_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 20706_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20706_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:32.77 +52:24:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.794 1028629755265754880 127.88631203383 +52.41544058884 12.2786 11.8208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20715_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20715_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:26.51 +54:42:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.281 1033598929347811712 127.11059208964 +54.71104373246 12.3939 11.7539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20719_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20719_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:48.66 +53:35:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.447 1028988303431757568 127.95266237033 +53.58680393706 12.3286 11.8032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20720_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20720_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:18:09.68 +54:10:19.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20721_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20721_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:12.58 +55:14:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.216 1030707454285323008 129.05248260849 +55.24849120167 12.3867 11.8977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20722_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20722_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:29:46.15 +54:04:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.637 1029068121103997440 127.44257160581 +54.07215654991 12.4680 12.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20727_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20727_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:24.43 +50:00:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.431 931892557590355456 126.10190453586 +50.01409539275 12.1682 11.7406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20731_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20731_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:42:29.54 +53:56:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.455 1030351526051764096 130.62311462682 +53.93784717628 12.2107 11.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20733_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20733_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:13:28.20 +54:08:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.800 1032629714143727744 123.36737844618 +54.13390072687 12.4679 12.0402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20735_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20735_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:30:58.12 +54:18:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.608 1030569912252566400 127.74234697958 +54.30995133770 12.5385 11.9942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20736_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20736_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:33:15.12 +54:28:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.295 1030589982635105152 128.31304964823 +54.47220105515 12.5177 12.0623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20739_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20739_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:43.57 +53:46:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.563 1028999092389602048 127.93131637784 +53.78075108240 12.7248 12.2436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20740_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20740_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:34:18.19 +55:27:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.111 1033728332418276096 128.57631894988 +55.46542322810 12.4951 11.9848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20741_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20741_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:33:51.19 +53:44:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.887 1030484532598167808 128.46328923234 +53.73364259174 12.5520 12.1692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20742_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20742_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:27.26 +53:34:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.552 1030283321970551296 129.11355483329 +53.57770788799 12.4320 11.9594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20743_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20743_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:34:09.09 +55:11:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.429 1030716082874834688 128.53793634184 +55.19458620582 12.4562 11.9840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20745_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20745_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:17.54 +53:05:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.392 1028904461373878144 126.82317895284 +53.09543528128 12.4945 11.9695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20747_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20747_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:42:03.51 +54:32:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.327 1030453501458802432 130.51472504051 +54.54995879098 12.2881 11.6095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20748_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20748_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:14:54.87 +53:42:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.228 1031834075746291712 123.72836906070 +53.70763870428 12.4638 11.7841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20750_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20750_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:40:19.90 +53:46:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.233 1030263049724881536 130.08301683663 +53.76710925996 12.5050 12.1005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20751_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20751_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:49:42.76 +54:24:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.681 1029976760088920192 132.42841765460 +54.40621331846 12.3215 11.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20752_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20752_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:19.23 +54:52:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.306 1032162383046379648 126.58017723523 +54.88116280307 12.4239 11.7466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20753_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20753_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:51.30 +53:01:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.514 1028902915185652992 126.71390633500 +53.03166309556 12.5290 12.0608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20754_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20754_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:55.90 +53:13:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.189 1031957775100322048 125.48299979167 +53.21790556964 12.5652 12.0301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20755_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20755_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:08:40.16 +55:04:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.323 1032921183508520448 122.16724438815 +55.06932372928 12.5886 12.1373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20759_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20759_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:30:56.20 +54:32:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.475 1030582526571831552 127.73435561049 +54.54223187606 12.6232 12.2191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20760_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20760_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:38:18.42 +54:16:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.827 1030428663664381824 129.57692937298 +54.27345434067 12.4793 11.9067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20761_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20761_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:32:40.50 +54:57:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.591 1030618157620471296 128.16872288974 +54.95327441918 12.5645 12.1295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20762_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20762_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:51.00 +54:46:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.247 1033600479831897984 127.21249649545 +54.77920910719 12.5854 12.1243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20763_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20763_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:19.30 +54:29:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.815 1030581255261587200 127.83051718144 +54.49133674032 12.6079 12.1404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20764_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20764_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:18.67 +55:22:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.182 1033700084417958528 127.07811956203 +55.37796478635 11.9183 10.7946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20766_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20766_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:32:51.02 +53:41:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.185 1028995587696278144 128.21256641286 +53.69478281856 12.6141 12.0584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20767_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20767_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:35:27.59 +54:42:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.500 1030643996143786624 128.86508458004 +54.71559049400 12.5137 11.9126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20768_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20768_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:45:12.16 +53:49:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.299 1029607294119251200 131.30080403393 +53.82082308687 12.4604 12.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20769_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20769_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:05.27 +52:22:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.190 1028810697944072960 126.77196498054 +52.37419143708 12.5413 11.9903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20771_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20771_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:11.41 +54:21:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.321 1030527001234713216 129.29751453744 +54.35233766640 12.5074 11.8552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20772_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20772_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:38:03.59 +54:44:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.361 1030634817798018688 129.51494863108 +54.74979468486 12.6120 12.1201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20773_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20773_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:57.01 +53:49:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.444 1032035153230944128 126.73773877473 +53.82584753880 12.6873 12.2481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20774_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20774_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:35:59.69 +52:10:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.468 1027902393964697088 128.99885355030 +52.17387737774 12.4984 12.0052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20775_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20775_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:07.58 +53:52:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.455 1032041200544895104 126.78173992146 +53.88049717142 12.6455 12.1566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20776_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20776_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:06.71 +54:52:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.582 1030646848002064384 129.02836998462 +54.87512004488 12.5800 12.0525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20778_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20778_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:01.65 +53:02:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.055 1028938584890432128 127.75657654150 +53.04375938614 12.5345 11.9428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20779_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20779_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:40:44.92 +52:57:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.123 1029453564353145984 130.18719903616 +52.96036149904 12.4175 11.7758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20781_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20781_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:43.37 +55:07:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.114 1032357134043453184 126.18074122634 +55.11952994941 12.5548 11.9434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20782_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20782_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:30:18.29 +54:36:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.319 1033580413744683520 127.57621691222 +54.60221696834 12.6733 12.2261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20783_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20783_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:57.09 +54:47:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.407 1032325355581257344 125.73792108928 +54.79219557365 12.6214 12.0896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20784_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20784_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:39:19.70 +56:06:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.099 1031166092369531264 129.83213167063 +56.10677172687 12.5795 12.1651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20785_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20785_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:23.13 +55:50:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.217 1033800968905159296 127.84638427177 +55.83666230794 12.6410 12.2033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20786_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20786_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:12:47.51 +53:52:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.105 1032601401719320064 123.19792543732 +53.87618855876 12.3522 11.6038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20787_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20787_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:19.13 +55:49:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.397 1033948058649414656 125.57984213838 +55.82369194798 12.6640 12.2525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:32:31.00 +55:46:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.226 1033751147284514176 128.12917935038 +55.77640991738 12.6316 12.1976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20790_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20790_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:03.50 +54:11:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.277 1030336717003897856 129.26468795507 +54.18921335013 12.6294 12.1269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20791_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20791_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:26.37 +53:38:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.334 1031937777732501504 126.36003149041 +53.64900332742 12.6368 12.0600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20792_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20792_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:41:23.07 +54:18:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.189 1030397499381658880 130.34616344672 +54.31621412493 12.5940 12.1242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20795_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20795_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:45.60 +56:32:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.141 1034052516549930880 127.18998392449 +56.53451730391 12.6597 12.1587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20796_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20796_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:36.26 +53:05:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.593 1028719335399336448 129.15084564749 +53.09094536490 12.6152 12.0901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20797_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20797_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:18:14.36 +55:56:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.500 1033210904822430080 124.55982978780 +55.93986113445 12.5887 12.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20798_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20798_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:49.95 +53:22:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.406 1031917127529812992 125.95827167821 +53.38084895055 12.6272 12.1463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20799_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20799_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:23.34 +54:11:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.533 1030335819354735104 129.34709232223 +54.18403239826 12.6574 12.1766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20801_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20801_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:09.93 +55:33:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.426 1033706479624662400 127.04137370773 +55.56395174469 12.6238 12.0004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20802_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20802_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:27.70 +57:35:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.409 1035268507690876160 126.86540970260 +57.59799754951 12.3686 11.6621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20803_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20803_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:30:41.21 +53:50:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.902 1029044515963691264 127.67156857363 +53.83656905420 12.7060 12.2913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20805_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20805_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:41:08.49 +53:32:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.357 1030245010862236032 130.28547132891 +53.53702556409 12.6379 12.1553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20806_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20806_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:16:50.42 +54:40:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.349 1032296665199633792 124.21023110643 +54.68140680436 12.6457 12.1884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20807_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20807_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:58.34 +53:00:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.156 1030203847895765760 129.49301619992 +53.01640490572 12.5957 12.1178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20809_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20809_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:44:16.78 +54:31:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.147 1030766896633031424 131.06998658138 +54.51813328891 12.6106 12.1486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20810_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20810_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:51:30.09 +55:12:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.061 1030144366892559744 132.87584614545 +55.21550952056 12.2662 11.4540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20811_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20811_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:44:26.45 +54:22:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.186 1030387260179596544 131.11028528299 +54.37564082568 12.5867 12.1855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20813_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20813_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:40.85 +53:36:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.339 1031937434135116928 126.42033064491 +53.60349548378 12.6832 12.1753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20815_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20815_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:26.45 +53:50:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.892 1032037932074278016 126.86052853287 +53.83397871282 12.7445 12.2692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20816_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20816_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:52.59 +55:38:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.381 1033707922733647616 126.96922703248 +55.64489429797 12.6252 12.0342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20817_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20817_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:49:23.03 +54:20:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.378 1029974973382526464 132.34613142814 +54.33913789740 12.5188 12.0401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20818_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20818_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:41.71 +53:06:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.410 1028915151548577152 126.67374196596 +53.10491550666 12.7217 12.2913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20819_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20819_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:51.83 +55:09:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.327 1032357688094999296 126.21593575989 +55.16013226238 12.7650 12.2126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20820_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20820_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:54:10.54 +55:13:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.339 1030120972206915328 133.54406295142 +55.22993262744 12.4896 11.9808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20821_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20821_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:07.95 +53:20:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.751 1031960249001480448 125.53332214659 +53.33656118688 12.6904 12.1664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20822_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20822_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:26.64 +53:32:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.931 1031968289180198400 125.61131667973 +53.53362163237 12.7499 12.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20824_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20824_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:46:50.37 +53:51:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.048 1029564207007315328 131.70985893379 +53.86020387572 12.5991 12.1432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20825_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20825_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:51.70 +54:17:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.917 1030558814057074176 127.96548628236 +54.29458184441 12.6051 11.8827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20827_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20827_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:58.91 +54:51:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.068 1032337622007862528 125.49547461319 +54.85784480681 12.6049 11.9161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20828_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20828_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:34:52.40 +54:16:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.519 1030534457297954176 128.71855232289 +54.27393331362 12.7027 12.2790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20829_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20829_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:40:33.61 +52:08:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.383 1027869133737300736 130.14017947519 +52.14885204453 12.5999 12.0344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20830_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20830_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:42:59.18 +52:17:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.328 1029363924091279360 130.74673168193 +52.29810169969 12.4966 11.9004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20831_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20831_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:38:55.54 +56:30:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.251 1034184183067723648 129.73152962961 +56.51363514240 12.6305 12.1762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20832_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20832_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:17.38 +52:56:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.346 1031526251146465024 125.32248216983 +52.94942086282 12.7144 12.2609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20833_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20833_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:38.73 +56:25:38.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 20834_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20834_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:21.55 +54:39:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.218 1032328104360342912 125.33984130030 +54.65241886585 12.7209 12.2261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20837_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20837_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:45.53 +54:52:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.280 1032159707282424960 126.18979141031 +54.86699416302 12.7012 12.1167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20838_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20838_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:55.85 +52:51:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.245 1028698543461778176 129.48276525624 +52.85337823834 12.5371 11.8664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20839_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20839_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:41:53.30 +52:37:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.511 1029385742525113088 130.47229272217 +52.61990886578 12.6226 12.1205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20840_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20840_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:54.71 +56:09:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.491 1033972664517671936 126.47820144385 +56.15970492879 12.6530 12.1412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20841_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20841_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:15:47.45 +54:12:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.391 1032257873055102464 123.94767356002 +54.21336545918 12.6390 12.0602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20842_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20842_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:29.82 +57:08:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.641 1034120995508390016 127.12445263103 +57.14172090207 12.7813 12.4262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20843_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20843_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:52.03 +53:44:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.384 1031986839143263744 125.46691419836 +53.73555045307 12.6707 12.1509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20845_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20845_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:03.76 +53:28:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.420 1031930356029071488 126.26583209870 +53.47574297194 12.6649 12.0477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20846_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20846_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:43.80 +52:50:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.405 1028885872755627264 126.18253125444 +52.84513881465 12.7087 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20848_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20848_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:42:52.36 +52:33:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.122 1029371311435026432 130.71821662813 +52.55070954283 12.6126 12.2030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20849_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20849_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:44:34.30 +53:30:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.250 1029575717519758848 131.14302920292 +53.51540777804 12.6237 12.1542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20850_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20850_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:42.08 +54:45:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.296 1032160222678495104 126.42541865688 +54.76189926282 12.6922 12.0768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20851_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20851_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:25.13 +53:16:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.501 1031959012050905728 125.35493904970 +53.27325992441 12.7472 12.3056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20852_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20852_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:08:02.15 +56:54:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.255 1081571927337805952 122.00908597122 +56.90218216776 12.5320 12.0300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20853_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20853_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:39.08 +53:42:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.294 1031939461359678976 126.41296507370 +53.70772528959 12.7564 12.3162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20854_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20854_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:46:39.20 +53:55:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.445 1029611520367049216 131.66353693583 +53.92769246020 12.4967 11.8373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20855_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20855_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:47.11 +53:30:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.217 1030232950594095232 129.44614047285 +53.50235352921 12.4224 11.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20856_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20856_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:32.91 +53:07:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.270 1031895785836607616 125.88723668307 +53.12752166206 12.7685 12.3622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20857_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20857_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:30:17.57 +52:31:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.499 1028640823396943104 127.57343418557 +52.52295468362 12.6504 12.1553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20859_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20859_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:06.41 +54:33:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.280 1032131424922117120 126.02673172740 +54.56522905579 12.8039 12.3366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20861_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20861_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:45:04.22 +53:54:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.330 1029608840307478016 131.26773414489 +53.90938336180 12.5096 11.8257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20862_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20862_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:40:18.45 +54:51:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.229 1030469964069809024 130.07688984970 +54.85907589872 12.7223 12.2639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20863_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20863_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:14:50.52 +53:34:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.215 1031830845930888704 123.71057784509 +53.57101755352 12.6567 12.0606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20864_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20864_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:38.49 +54:02:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.238 1032009452146708224 125.91047004552 +54.04302000640 12.7632 12.2642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20865_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20865_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:39:05.24 +55:43:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.528 1031117164102164096 129.77202008178 +55.72195334357 12.7912 12.2685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20866_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20866_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:45:52.29 +55:54:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.323 1030993945783448576 131.46801328435 +55.90598988786 12.5530 12.0275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20867_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20867_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:48:17.24 +56:18:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.197 1031034288412611584 132.07193150896 +56.31636678526 12.5673 12.0539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20868_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20868_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:15:11.41 +53:50:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.188 1031858578535349760 123.79762006944 +53.83483676046 12.6669 12.1387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20870_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20870_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:24.35 +56:24:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.496 1033854290923654784 127.85168038506 +56.40893765413 12.7121 12.2368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20872_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20872_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:59.23 +56:23:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.647 1034739569582780544 125.74700589486 +56.39589278545 12.7304 12.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20874_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20874_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:16.75 +53:33:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.242 1028989609101822976 127.81973182838 +53.56086272550 12.6454 11.9997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20875_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20875_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:35:23.37 +56:16:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.347 1034160337409384064 128.84748652672 +56.27414848547 12.7125 12.2449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20876_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20876_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:17:05.02 +54:55:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.403 1033057149288901760 124.27110565746 +54.92938988440 12.6635 12.0971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20877_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20877_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:47.36 +52:07:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.051 1028431125913998720 126.69735626872 +52.13244246792 12.6703 12.0329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20878_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20878_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:41:17.16 +52:53:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.486 1029440404573352704 130.32171996954 +52.88521923104 12.6451 12.1727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20879_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20879_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:37:43.22 +56:29:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.341 1034180437856254720 129.42996458883 +56.48962598747 12.8500 12.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20880_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20880_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:47:34.95 +53:40:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.355 1029558498993766784 131.89568058043 +53.68325968660 12.5395 11.9695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20881_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20881_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:09.65 +55:36:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.143 1033706891941495424 127.04018764613 +55.60790658492 12.6841 11.9819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20882_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20882_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:39.36 +53:16:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.873 1030269470700433536 129.16375038203 +53.26874648882 12.7038 12.1602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20884_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20884_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:53.05 +53:46:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.847 1029034448560364928 126.97064923478 +53.78028998188 12.9409 12.1973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20885_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20885_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:33:00.35 +54:23:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.987 1030566201400820864 128.25165046892 +54.39858304594 12.7747 12.2346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20886_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20886_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:36:39.44 +56:54:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.610 1034254654891074304 129.16490804704 +56.90776471373 12.9842 12.4641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20887_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20887_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:37.92 +53:21:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.258 1028949305128767104 127.90790493483 +53.36612294356 12.7605 12.3068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20888_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20888_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:00:39.65 +54:22:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.234 1032825117975860352 120.16522351947 +54.36943567142 12.5610 11.8966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20889_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20889_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:14:50.51 +55:22:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.428 1033128136508284672 123.71038842101 +55.37838786830 12.6259 11.9997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20890_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20890_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:47:04.77 +55:31:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.181 1030925883438168576 131.76996173527 +55.52360081355 12.6676 12.1667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20891_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20891_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:24.39 +54:55:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.662 1033651843344893952 126.85177282151 +54.92580200576 12.8347 12.3673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20892_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20892_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:53.11 +56:43:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.478 1034095603661811712 126.47147543922 +56.71666382654 12.6776 12.2019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20893_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20893_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:38:26.65 +56:12:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.301 1031148019147104128 129.61118724418 +56.21228470588 12.7104 12.3097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20894_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20894_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:18:43.22 +54:11:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.105 1032200591075847552 124.68012781578 +54.18468128750 12.6791 12.0884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20895_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20895_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:48.43 +55:56:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.308 1033908407511837696 126.95186267151 +55.93675745431 12.7369 12.2000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20896_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20896_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:20:22.52 +52:38:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.195 1031496907929959808 125.09392245504 +52.64324887383 12.6121 11.8934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20897_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20897_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:26:54.69 +51:27:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.145 1028189233355729280 126.72781364708 +51.45065163154 12.5954 12.0356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20898_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20898_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:29:42.88 +55:09:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.477 1033635251887079680 127.42876978965 +55.15222991715 12.8294 12.4467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20899_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20899_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:27:27.06 +51:50:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.277 1028406936658232448 126.86279279562 +51.84584997204 12.6785 12.1820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20901_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20901_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:34:24.36 +54:07:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.092 1030508928012357504 128.60178790158 +54.12252560406 12.7952 12.3779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20902_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20902_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:14:27.64 +53:25:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.510 1031824046998352896 123.61535083096 +53.43221595910 12.4961 11.6592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20903_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20903_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:34:14.84 +52:01:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.387 1028558703622293120 128.56199733772 +52.03114827863 12.6694 12.2236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20904_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20904_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:30.08 +51:58:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.435 1028461534282445824 125.37546886101 +51.97908740697 12.7091 12.2989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20905_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20905_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:25:15.13 +54:20:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.244 1032112290843509760 126.31311219098 +54.34566510749 12.7987 12.2185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20906_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20906_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:33:32.82 +53:34:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.917 1028979369899764992 128.38645423751 +53.58023993639 12.7899 12.2130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20908_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20908_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:11:29.09 +55:23:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.983 1033117721212599552 122.87144725349 +55.39015357852 12.5582 11.8823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20909_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20909_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:32:34.64 +53:35:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.189 1028981740721720192 128.14430941244 +53.59342164241 12.9719 12.4750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20910_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20910_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:50.58 +54:52:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.671 1032346624259300096 125.96081466994 +54.86862304411 12.7789 12.2802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20913_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20913_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:19:44.60 +55:23:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.589 1032413591389311360 124.93568898320 +55.39252498901 12.6991 12.1127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20916_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20916_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:34.73 +54:35:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.046 1032313707629957504 125.64503351562 +54.59047309501 12.8185 12.3014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20917_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20917_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:24:36.92 +54:57:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.227 1032353771084877696 126.15392920007 +54.96422526453 12.7279 12.0810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20918_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20918_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:26.79 +53:48:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.281 1031996979561722880 125.86164183761 +53.80910510214 12.7942 12.3034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20919_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20919_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:23:19.24 +52:27:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.150 1028498883317983104 125.83022712529 +52.46532482700 12.7175 12.2376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20925_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20925_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:22:36.28 +54:19:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.284 1032121739771575424 125.65122551781 +54.32606788917 12.7043 11.9904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20926_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20926_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:40:49.52 +50:08:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.437 1027399234251398144 130.20629849273 +50.13662936605 10.8545 9.5429 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20930_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20930_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:55.47 +53:37:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.686 1028988818827830528 127.98104914537 +53.63270379994 12.7696 12.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20931_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20931_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:33:57.00 +53:14:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.012 1028777678235022720 128.48709903406 +53.24200755185 12.7641 12.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20932_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20932_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:38:05.80 +52:26:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.931 1027932944067207808 129.52424745925 +52.44457948362 12.6447 12.0819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20942_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20942_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:21:34.24 +52:06:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.465 1028463286629101056 125.39287011824 +52.10400512281 12.6906 12.1638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 20946_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 20946_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:31:23.16 +51:22:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.230 1028139613597884288 127.84645541478 +51.37888698582 12.5840 11.9061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 26s
Prepared the HTML report for the field Lyn-02-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 ####
07:33:26.27 +57:47:50.2
08:04:35.78 +56:21:35.4
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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:14.834 +54:00:07.16
Angular distance between the image centers 0.08 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 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:13.865 +54:00:35.63
Angular distance between the image centers 0.08 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 08:28:14.834 +54:00:07.16
Second-epoch second image center 08:28:13.865 +54:00:35.63
Angular distance between the image centers 0.00826 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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.73kqfO8KhD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.pL6nAdMsjc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.jnkZ8UIKGQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.LM1XPx0ogX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits) and catalog (wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat) found
'wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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 29 out of 62506 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.714976
a=0.000000 b=1.000000 c=21.714976
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.53
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 206 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
1.9 pix Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
2.3 pix Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
2.3 pix Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Limiting magnitude estimates:
14.5 mag. Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
14.5 mag. Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
14.4 mag. Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
14.4 mag. Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.73kqfO8KhD (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/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3425, passed=62483
Got 62483 stars (including 58942 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
util/solve_plate_with_UCAC5 got 62483 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 166 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: 10.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.53"
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 213 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.44"
Estimated accuracy of the plate solution: 7.02"
Excluding outliers - 183 stars left (next iteration limit 141)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits -region wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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.pL6nAdMsjc (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/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3444, passed=62607
Got 62607 stars (including 59048 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
util/solve_plate_with_UCAC5 got 62607 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.3'
Seting catalog search parameters based on the expected field of view 927.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012879 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010303 (37.1 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 169 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: 9.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.89"
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 213 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.88"
Estimated accuracy of the plate solution: 7.17"
Excluding outliers - 187 stars left (next iteration limit 143)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits -region wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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.jnkZ8UIKGQ (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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=4123, passed=58681
Got 58681 stars (including 54493 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 58681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-30-09_20.00sec_-15.00C_LIGHT_0228.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.LM1XPx0ogX (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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=4196, passed=58338
Got 58338 stars (including 54075 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 58338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Lyn-02-Q2b1x1_003149_TTUQ2b1x1_14282_ehfnnHk9/Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229.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 Lyn-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out77046.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out77624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78090.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out78137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78215.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out78380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78521.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out78786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79063.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out43910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77054.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77065.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77103.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77111.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77154.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77180.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out78895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79172.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 207s
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: 93s
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Considering the candidate 77046_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77046_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:35:54.37 +54:32:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.097 985508631507838848 113.97628739467 +54.54526671834 14.0376 13.4844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77048_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77048_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 09:12:50.95 +49:49:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.132 1013079813286458752 138.21181873487 +49.82054782904 14.2016 13.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77051_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77051_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:37:53.27 +54:42:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.603 985596764236413952 114.47076836826 +54.70249832317 14.0614 13.6400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77052_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77052_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 77054_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77054_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77056_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77056_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77058_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77058_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:37:01.25 +58:16:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.785 1085428606107697536 114.25433063000 +58.27882337913 13.8832 13.3216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:45:50.20 +57:41:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.890 1082419517660046976 116.46115573257 +57.68485920422 13.9611 13.3853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77065_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77065_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77067_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77067_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:20:14.53 +49:02:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.704 931792162730890112 125.06070191540 +49.04163721837 14.4279 13.5071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77072_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77072_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 77076_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77076_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:37:31.17 +54:31:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.060 985587349668104832 114.37898306423 +54.52207708603 14.1032 13.6261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77077_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77077_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 77078_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77078_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:37:34.05 +55:58:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.838 986114050097298432 114.39260582460 +55.98145168431 13.4800 12.8245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77079_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77079_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77080_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77080_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77084_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77084_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:35:57.27 +53:50:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.867 985453518487582720 113.98857358863 +53.84484430083 14.0093 13.5232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77093_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77093_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:43:28.88 +58:05:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.335 1082492768325994240 115.87303875922 +58.08588776732 13.6597 13.1408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77094_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77094_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 77095_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77095_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:38:16.48 +54:52:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.273 985621675046674816 114.56853152726 +54.86884948360 14.1131 13.6551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77097_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77097_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:40:56.58 +56:32:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.876 986201770509443072 115.23438095929 +56.54382335762 14.0161 13.4662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77099_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77099_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77103_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77103_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77104_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77104_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:52:49.15 +58:38:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.996 1037497939315902208 133.20472559031 +58.64122538139 14.6703 14.1664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77106_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77106_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77108_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77108_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:35:23.23 +55:48:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.712 986097282545001472 113.84583840008 +55.81424800475 13.5040 12.8520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77109_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77109_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77111_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77111_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77113_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77113_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:38:44.42 +56:56:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.397 986272993950830336 114.68627025499 +56.94187764040 13.6425 13.1658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77114_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77114_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77119_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77119_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 77120_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77120_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:46:55.52 +58:31:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.751 1082853996552003968 116.73381213001 +58.52804707300 13.7742 13.3179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77130_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77130_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:08.66 +58:04:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.520 989570605418256000 112.78370960905 +58.07266531638 13.0732 12.3555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77133_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77133_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:46.90 +56:58:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.829 989263841673632384 113.69736684220 +56.97348887172 13.1548 12.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77134_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77134_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:33:34.15 +58:29:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.243 1085471933737751808 113.39311153669 +58.48456335428 13.0172 12.2670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77138_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77138_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:35:50.57 +55:51:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.459 986085943831334144 113.96109746288 +55.85592485239 13.3996 12.7226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77144_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77144_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:40:55.05 +58:31:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.360 1085520449688541696 115.23049813091 +58.52681795149 13.5367 12.9121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77149_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77149_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:22.96 +58:00:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.924 1085399361673764352 114.09466285491 +58.00430252013 13.3827 12.7821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77154_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77154_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77161_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77161_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:23.10 +56:50:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.832 989246799243386496 114.09768755794 +56.84485943856 13.3554 12.8345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77162_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77162_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:42:59.09 +57:31:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.199 1082332415722988032 115.74776433885 +57.53058114273 13.4130 12.7796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77167_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77167_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:40:31.32 +56:29:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.130 986180742349568000 115.13098541799 +56.48808304365 13.4206 12.8283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77169_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77169_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77171_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77171_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:52.08 +53:47:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.031 985265776877132672 114.21842402806 +53.78661640963 13.4895 12.8891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77172_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77172_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77173_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77173_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:41:14.02 +56:01:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.796 986149578066909696 115.30712902813 +56.02009678984 13.4771 12.7949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77176_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77176_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 77179_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77179_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:19.71 +54:16:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.717 985492310632117248 114.08477073833 +54.27308955087 13.2348 12.5507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77180_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77180_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77181_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77181_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:35:44.30 +56:17:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.520 986136860667662208 113.93617690492 +56.29125013796 13.3274 12.8325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77184_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77184_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77186_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77186_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:39:41.85 +58:32:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.280 1085522854870238848 114.92210688323 +58.54324828247 13.0015 12.4134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77187_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77187_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77190_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77190_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:40:04.29 +57:18:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.052 1082349733031265280 115.01932269574 +57.30779956376 13.0787 12.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77192_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77192_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77193_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77193_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 77195_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77195_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 77197_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77197_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77198_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77198_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:01.55 +55:16:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.501 985693005863459456 114.00905226464 +55.26994466089 13.0534 12.3105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77200_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77200_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77202_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77202_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77210_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77210_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77211_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77211_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:08.67 +57:01:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.758 989256248171435520 114.03475512050 +57.01970325432 12.9218 12.3326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77213_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77213_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:58:12.20 +48:35:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.540 1015633188524156032 134.55086197041 +48.59234312732 13.9246 13.4823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77215_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77215_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:42:17.55 +58:08:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.112 1082502805665806208 115.57053731264 +58.13491557093 12.9117 12.2514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77217_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77217_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:33:00.38 +57:06:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.294 989315037683755904 113.24989927861 +57.10661373244 12.8157 12.1028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77218_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77218_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:04:40.25 +52:42:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.258 936404236051932800 121.16809800487 +52.70575755477 13.9394 13.2799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77219_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77219_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:46.06 +55:55:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.364 986101813734508288 113.69235335442 +55.92940060183 12.9408 12.3616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77220_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77220_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 77226_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77226_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77228_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77228_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 77230_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77230_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77234_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77234_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:39:21.65 +58:11:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.823 1085418195106949760 114.83873350458 +58.19900579709 12.7648 12.2614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77237_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77237_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:53.27 +57:17:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.119 989283358004998016 114.21999596265 +57.29284823226 12.3478 11.7276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77239_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77239_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77243_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77243_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:08.38 +55:53:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.009 986100748582620288 113.53487868848 +55.89658488809 12.2609 11.5914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77244_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77244_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77245_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77245_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:17.87 +56:23:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.530 989142788019429376 113.57665145066 +56.38583092842 12.1793 11.4856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77247_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77247_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 77257_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77257_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 77260_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77260_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77261_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77261_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77262_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77262_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:32.25 +55:31:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.910 985711044726060032 113.63202372048 +55.52772976603 11.7804 11.1244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77266_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77266_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77267_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77267_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77270_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77270_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77271_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77271_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77275_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77275_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 77276_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77276_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77277_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77277_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:33:15.60 +56:26:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 4.470 989132312594780416 113.31689308033 +56.43566779535 11.0042 10.3264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77278_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77278_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:33.69 +57:47:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 4.073 1085388645732080256 114.13825218974 +57.79000590256 10.4666 9.7857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77279_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77279_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77280_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77280_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:04.58 +56:15:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 2.266 989115510682715008 113.51806526241 +56.25544334052 10.1400 9.4177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77281_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77281_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77282_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77282_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:40:54.56 +58:08:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.88, MAG_FAINT_SEARCH_LIMIT=10.86)GAIADR2_OUTPUT=# 3.764 1082505623164363008 115.22930548783 +58.14962780012 9.8556 9.1932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77283_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77283_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:36:48.42 +56:51:26.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 77394_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77394_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77520_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77520_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77521_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77521_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:32:11.86 +57:06:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 3.575 989224735994807040 113.05124466083 +57.11631049017 11.6037 11.1833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77538_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77538_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 77548_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77548_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:38.44 +58:26:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 5.524 1085656342453902208 112.91305319503 +58.44749271381 11.3314 10.6147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77560_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77560_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:32:33.11 +56:57:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.466 989219895567780608 113.13866671246 +56.95110072842 11.6432 10.9773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77613_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77613_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77624_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77624_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:35.69 +58:05:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.563 989570257523837952 112.90000827061 +58.08949150019 11.6920 11.0254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77651_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77651_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77676_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77676_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:33:25.89 +58:01:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 4.441 1085455780364968192 113.36019924989 +58.02458272308 12.1199 11.5605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77723_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77723_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77757_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77757_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77843_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77843_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77901_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77901_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77926_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77926_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:18.63 +58:02:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.904 989569742127765760 112.82860248826 +58.04558180321 12.7023 12.1975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 77949_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 77949_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 77950_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 77950_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:32:54.79 +58:14:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.128 1085462583593167744 113.22941040348 +58.24408632753 12.6248 12.0930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78049_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78049_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:30.69 +58:21:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.457 1085467222157857792 113.63060460941 +58.35294065707 12.8029 12.1066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78076_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78076_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78090_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78090_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:27.77 +57:52:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.469 989362518545663232 113.61797555846 +57.86712827592 12.7988 12.2097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78121_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78121_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:32:37.29 +57:58:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.927 989379393473550080 113.15690770114 +57.97914039399 12.9952 12.4945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78137_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78137_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:33:39.46 +57:00:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.299 989266624812450048 113.41703314452 +57.00231295344 13.0248 12.6062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78138_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78138_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:09.23 +58:06:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.795 989571223893545088 112.79043835836 +58.11199178101 12.8683 12.3232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78153_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78153_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78158_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78158_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78165_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78165_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78215_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78215_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:44.42 +58:03:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.681 989569952583223296 112.93596087599 +58.05585389581 13.3174 12.8653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78222_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78222_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:32:18.34 +58:20:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.670 1085652013126845824 113.07833362611 +58.33566252471 12.9851 12.3061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78240_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78240_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78287_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78287_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78352_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78352_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78364_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78364_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 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 78379_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78379_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78380_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78380_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:28:58.33 +51:44:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.177 1028209746119485696 127.24290109211 +51.73720707883 14.0777 12.9869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78417_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78417_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78447_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78447_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78489_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78489_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78509_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78509_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78521_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78521_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:37.72 +58:07:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.643 1085451420974009600 113.65908107315 +58.11851150041 13.3145 12.7394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78532_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78532_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78547_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78547_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:31:44.37 +58:25:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.095 1085656170653780608 112.93704574219 +58.42331813168 13.5665 12.9640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78557_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78557_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78569_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78569_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78595_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78595_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78600_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78600_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78671_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78671_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 78675_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78675_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78699_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78699_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78711_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78711_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78715_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78715_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78739_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78739_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78754_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78754_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78775_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78775_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78777_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78777_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78779_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78779_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78786_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78786_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:54:18.63 +56:45:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.225 1081385117736681216 118.57783134906 +56.75694094044 14.6459 13.6265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78789_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78808_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78808_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78826_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78826_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78829_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78829_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78830_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78830_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78855_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78855_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78862_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78862_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78863_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78863_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78868_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78868_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78873_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78873_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78877_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78877_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:34:23.49 +58:02:40.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 78878_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78878_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78879_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78879_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78884_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78884_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78888_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78888_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78895_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78895_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78909_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78909_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78912_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78912_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78914_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78914_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78921_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 78921_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:46:08.50 +52:10:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.718 984320437394658560 116.53521158310 +52.18037702767 14.8445 14.3573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 78925_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78925_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78927_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78927_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
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Considering the candidate 78936_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78936_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78942_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78942_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78951_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78951_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78953_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78953_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78958_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78958_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78963_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78963_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78965_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78965_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78971_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78971_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78982_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78982_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78987_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 78987_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79003_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79003_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79027_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79027_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79030_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79030_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79031_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79031_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79034_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79034_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79062_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79063_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 79063_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:50:19.16 +51:47:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.029 984065316337066112 117.58027859340 +51.79452122336 15.0296 14.4749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79064_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79064_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79068_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 79068_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 07:47:30.90 +51:35:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.750 982604683858859648 116.87952953793 +51.58367838585 14.8484 14.3625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79073_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79073_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79132_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79132_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79134_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79134_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79153_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79153_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79172_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 79172_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43910_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 43910_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25559_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 25559_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02012_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 02012_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48208_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 48208_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50114_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
Preparing report for the candidate 50114_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16990_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229
The candidate 16990_Lyn-02-Q2b1x1_2026-02-22_00-31-02_20.00sec_-15.00C_LIGHT_0229 did not pass the final checks
**** FOUND 08:04:35.78 +56:21:35.4 in the exclusion list exclusion_list_local.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 15s
make_report_in_HTML.sh TOTAL: 315s
Prepared the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:33:26.27 +57:47:50.2
08:04:35.78 +56:21:35.4
08:11:21.13 +52:44:23.5
08:24:24.41 +50:00:50.4
08:40:49.50 +50:08:14.2
08:02:45.70 +52:44:30.0
08:00:48.23 +54:07:56.4
08:06:41.30 +53:24:12.5
07:37:35.15 +55:38:53.4
08:24:02.85 +58:57:22.6
07:37:02.08 +57:52:50.9
08:06:08.26 +49:02:14.8
08:29:05.31 +55:04:05.3
07:37:20.06 +57:39:30.5
08:04:31.04 +51:21:15.9
07:35:54.59 +56:58:53.8
07:39:49.02 +58:29:22.2
07:44:21.68 +58:41:28.8
08:16:03.36 +58:22:27.0
07:35:45.61 +58:16:49.4
07:37:54.68 +57:19:53.7
08:07:56.59 +55:02:27.2
07:32:11.36 +58:27:05.4
07:39:33.22 +57:53:54.5
07:35:17.46 +58:24:10.8
07:34:57.58 +56:29:31.9
07:37:47.10 +56:47:51.1
07:49:58.73 +51:44:41.7
07:35:30.82 +57:28:50.8
07:33:30.92 +56:35:02.6
07:33:35.43 +55:55:45.6
07:32:48.15 +56:59:29.8
08:03:46.18 +57:19:10.9
07:37:56.32 +58:12:07.0
07:34:42.45 +56:39:57.9
07:36:18.42 +57:09:53.8
09:10:28.33 +52:41:21.2
07:40:34.93 +58:26:28.0
08:14:03.24 +49:24:37.9
07:34:19.47 +58:09:21.4
07:56:16.97 +53:45:57.2
07:31:05.44 +58:13:05.1
07:36:01.52 +56:32:38.1
07:58:44.51 +57:15:32.9
07:31:51.09 +57:58:09.5
07:32:49.55 +58:06:03.7
08:15:07.93 +55:00:04.7
07:36:11.73 +58:05:21.6
08:11:50.52 +49:33:53.3
07:33:03.73 +57:22:33.4
07:35:04.51 +58:01:16.1
07:58:10.51 +51:12:03.6
08:18:50.04 +56:16:22.1
08:17:21.05 +52:15:09.2
08:16:24.41 +49:29:13.6
08:29:48.66 +56:04:33.4
08:26:50.11 +48:55:55.6
07:34:44.72 +57:52:57.3
08:17:54.11 +50:08:08.5
08:59:43.33 +58:30:39.8
08:45:23.06 +55:11:44.6
07:34:44.80 +58:28:41.1
08:07:33.55 +49:02:17.8
07:52:49.62 +50:19:49.1
08:30:37.64 +51:06:21.3
08:38:01.66 +52:01:21.1
08:02:58.18 +53:38:06.6
08:13:01.44 +54:31:15.9
08:19:18.12 +55:55:20.4
08:21:42.68 +50:00:19.9
08:09:55.59 +55:33:44.5
08:17:42.83 +52:04:08.2
08:11:54.46 +53:41:57.4
08:20:13.67 +51:04:59.7
08:44:32.92 +55:38:03.2
08:17:46.23 +55:14:16.0
08:26:40.76 +52:16:14.3
08:43:33.11 +56:05:22.5
08:16:45.76 +51:28:12.0
08:32:27.42 +54:28:06.5
08:06:33.81 +54:30:34.0
07:53:14.38 +49:37:44.5
08:25:28.73 +52:13:37.8
08:08:36.56 +52:36:42.5
08:16:28.29 +49:57:20.4
08:48:00.70 +58:37:52.2
08:38:40.47 +55:51:14.8
08:12:02.65 +49:06:12.1
07:52:01.91 +53:28:17.2
08:16:50.27 +49:05:57.4
08:55:57.77 +54:37:03.4
08:07:40.69 +54:24:36.6
08:33:19.87 +52:03:06.8
08:16:47.27 +53:19:27.1
08:23:50.71 +49:51:51.7
08:04:39.72 +53:03:21.7
08:12:11.82 +52:10:51.4
08:06:32.76 +56:24:07.0
07:57:42.82 +52:17:01.7
08:17:41.87 +50:22:47.5
08:22:55.67 +54:34:22.5
08:39:14.67 +57:35:57.3
08:08:43.10 +55:33:31.6
07:47:52.93 +51:09:31.9
08:08:35.55 +51:53:33.5
07:51:48.53 +51:58:36.3
08:26:22.19 +54:32:23.8
08:10:40.42 +51:39:25.9
08:15:26.45 +52:32:07.1
08:06:23.34 +53:52:41.1
08:11:29.64 +52:51:13.0
07:52:58.50 +52:53:05.4
08:07:24.34 +50:18:18.2
07:54:25.44 +50:39:49.1
08:40:06.01 +49:52:55.7
08:09:20.71 +49:41:15.1
########### Completed Lyn-02-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 ####
07:33:26.27 +57:47:50.2
08:04:35.78 +56:21:35.4
08:02:45.70 +52:44:30.0
08:00:48.23 +54:07:56.4
08:06:41.30 +53:24:12.5
07:37:35.15 +55:38:53.4
08:24:02.85 +58:57:22.6
07:37:02.08 +57:52:50.9
08:06:08.26 +49:02:14.8
08:29:05.31 +55:04:05.3
07:37:20.06 +57:39:30.5
08:04:31.04 +51:21:15.9
07:35:54.59 +56:58:53.8
07:39:49.02 +58:29:22.2
07:44:21.68 +58:41:28.8
08:16:03.36 +58:22:27.0
07:35:45.61 +58:16:49.4
07:37:54.68 +57:19:53.7
08:07:56.59 +55:02:27.2
07:32:11.36 +58:27:05.4
07:39:33.22 +57:53:54.5
07:35:17.46 +58:24:10.8
07:34:57.58 +56:29:31.9
07:37:47.10 +56:47:51.1
07:49:58.73 +51:44:41.7
07:35:30.82 +57:28:50.8
07:33:30.92 +56:35:02.6
07:33:35.43 +55:55:45.6
07:32:48.15 +56:59:29.8
08:03:46.18 +57:19:10.9
07:37:56.32 +58:12:07.0
07:34:42.45 +56:39:57.9
07:36:18.42 +57:09:53.8
09:10:28.33 +52:41:21.2
07:40:34.93 +58:26:28.0
08:14:03.24 +49:24:37.9
07:34:19.47 +58:09:21.4
07:56:16.97 +53:45:57.2
07:31:05.44 +58:13:05.1
07:36:01.52 +56:32:38.1
07:58:44.51 +57:15:32.9
07:31:51.09 +57:58:09.5
07:32:49.55 +58:06:03.7
08:15:07.93 +55:00:04.7
07:36:11.73 +58:05:21.6
08:11:50.52 +49:33:53.3
07:33:03.73 +57:22:33.4
07:35:04.51 +58:01:16.1
07:58:10.51 +51:12:03.6
08:18:50.04 +56:16:22.1
08:17:21.05 +52:15:09.2
08:16:24.41 +49:29:13.6
08:29:48.66 +56:04:33.4
08:26:50.11 +48:55:55.6
07:34:44.72 +57:52:57.3
08:17:54.11 +50:08:08.5
08:59:43.33 +58:30:39.8
08:45:23.06 +55:11:44.6
07:34:44.80 +58:28:41.1
08:07:33.55 +49:02:17.8
07:52:49.62 +50:19:49.1
08:30:37.64 +51:06:21.3
08:38:01.66 +52:01:21.1
08:02:58.18 +53:38:06.6
08:13:01.44 +54:31:15.9
08:19:18.12 +55:55:20.4
08:21:42.68 +50:00:19.9
08:09:55.59 +55:33:44.5
08:17:42.83 +52:04:08.2
08:11:54.46 +53:41:57.4
08:20:13.67 +51:04:59.7
08:44:32.92 +55:38:03.2
08:17:46.23 +55:14:16.0
08:26:40.76 +52:16:14.3
08:43:33.11 +56:05:22.5
08:16:45.76 +51:28:12.0
08:32:27.42 +54:28:06.5
08:06:33.81 +54:30:34.0
07:53:14.38 +49:37:44.5
08:25:28.73 +52:13:37.8
08:08:36.56 +52:36:42.5
08:16:28.29 +49:57:20.4
08:48:00.70 +58:37:52.2
08:38:40.47 +55:51:14.8
08:12:02.65 +49:06:12.1
07:52:01.91 +53:28:17.2
08:16:50.27 +49:05:57.4
08:55:57.77 +54:37:03.4
08:07:40.69 +54:24:36.6
08:33:19.87 +52:03:06.8
08:16:47.27 +53:19:27.1
08:23:50.71 +49:51:51.7
08:04:39.72 +53:03:21.7
08:12:11.82 +52:10:51.4
08:06:32.76 +56:24:07.0
07:57:42.82 +52:17:01.7
08:17:41.87 +50:22:47.5
08:22:55.67 +54:34:22.5
08:39:14.67 +57:35:57.3
08:08:43.10 +55:33:31.6
07:47:52.93 +51:09:31.9
08:08:35.55 +51:53:33.5
07:51:48.53 +51:58:36.3
08:26:22.19 +54:32:23.8
08:10:40.42 +51:39:25.9
08:15:26.45 +52:32:07.1
08:06:23.34 +53:52:41.1
08:11:29.64 +52:51:13.0
07:52:58.50 +52:53:05.4
08:07:24.34 +50:18:18.2
07:54:25.44 +50:39:49.1
08:40:06.01 +49:52:55.7
08:09:20.71 +49:41:15.1
08:11:21.13 +52:44:23.5
08:24:24.41 +50:00:50.4
08:40:49.50 +50:08:14.2
###################################################################################
07:33:26.27 +57:47:50.2 -- not an asteroid (will add it to exclusion list)
08:04:35.78 +56:21:35.4 -- not an asteroid (will add it to exclusion list)
08:02:45.70 +52:44:30.0 -- not an asteroid (will add it to exclusion list)
08:00:48.23 +54:07:56.4 -- not an asteroid (will add it to exclusion list)
08:06:41.30 +53:24:12.5 -- not an asteroid (will add it to exclusion list)
07:37:35.15 +55:38:53.4 -- not an asteroid (will add it to exclusion list)
08:24:02.85 +58:57:22.6 -- not an asteroid (will add it to exclusion list)
07:37:02.08 +57:52:50.9 -- not an asteroid (will add it to exclusion list)
08:06:08.26 +49:02:14.8 -- not an asteroid (will add it to exclusion list)
08:29:05.31 +55:04:05.3 -- not an asteroid (will add it to exclusion list)
07:37:20.06 +57:39:30.5 -- not an asteroid (will add it to exclusion list)
08:04:31.04 +51:21:15.9 -- not an asteroid (will add it to exclusion list)
07:35:54.59 +56:58:53.8 -- not an asteroid (will add it to exclusion list)
07:39:49.02 +58:29:22.2 -- not an asteroid (will add it to exclusion list)
07:44:21.68 +58:41:28.8 -- not an asteroid (will add it to exclusion list)
08:16:03.36 +58:22:27.0 -- not an asteroid (will add it to exclusion list)
07:35:45.61 +58:16:49.4 -- not an asteroid (will add it to exclusion list)
07:37:54.68 +57:19:53.7 -- not an asteroid (will add it to exclusion list)
08:07:56.59 +55:02:27.2 -- not an asteroid (will add it to exclusion list)
07:32:11.36 +58:27:05.4 -- not an asteroid (will add it to exclusion list)
07:39:33.22 +57:53:54.5 -- not an asteroid (will add it to exclusion list)
07:35:17.46 +58:24:10.8 -- not an asteroid (will add it to exclusion list)
07:34:57.58 +56:29:31.9 -- not an asteroid (will add it to exclusion list)
07:37:47.10 +56:47:51.1 -- not an asteroid (will add it to exclusion list)
07:49:58.73 +51:44:41.7 -- not an asteroid (will add it to exclusion list)
07:35:30.82 +57:28:50.8 -- not an asteroid (will add it to exclusion list)
07:33:30.92 +56:35:02.6 -- not an asteroid (will add it to exclusion list)
07:33:35.43 +55:55:45.6 -- not an asteroid (will add it to exclusion list)
07:32:48.15 +56:59:29.8 -- not an asteroid (will add it to exclusion list)
08:03:46.18 +57:19:10.9 -- not an asteroid (will add it to exclusion list)
07:37:56.32 +58:12:07.0 -- not an asteroid (will add it to exclusion list)
07:34:42.45 +56:39:57.9 -- not an asteroid (will add it to exclusion list)
07:36:18.42 +57:09:53.8 -- not an asteroid (will add it to exclusion list)
09:10:28.33 +52:41:21.2 -- not an asteroid (will add it to exclusion list)
07:40:34.93 +58:26:28.0 -- not an asteroid (will add it to exclusion list)
08:14:03.24 +49:24:37.9 -- not an asteroid (will add it to exclusion list)
07:34:19.47 +58:09:21.4 -- not an asteroid (will add it to exclusion list)
07:56:16.97 +53:45:57.2 -- not an asteroid (will add it to exclusion list)
07:31:05.44 +58:13:05.1 -- not an asteroid (will add it to exclusion list)
07:36:01.52 +56:32:38.1 -- not an asteroid (will add it to exclusion list)
07:58:44.51 +57:15:32.9 -- not an asteroid (will add it to exclusion list)
07:31:51.09 +57:58:09.5 -- not an asteroid (will add it to exclusion list)
07:32:49.55 +58:06:03.7 -- not an asteroid (will add it to exclusion list)
08:15:07.93 +55:00:04.7 -- not an asteroid (will add it to exclusion list)
07:36:11.73 +58:05:21.6 -- not an asteroid (will add it to exclusion list)
08:11:50.52 +49:33:53.3 -- not an asteroid (will add it to exclusion list)
07:33:03.73 +57:22:33.4 -- not an asteroid (will add it to exclusion list)
07:35:04.51 +58:01:16.1 -- not an asteroid (will add it to exclusion list)
07:58:10.51 +51:12:03.6 -- not an asteroid (will add it to exclusion list)
08:18:50.04 +56:16:22.1 -- not an asteroid (will add it to exclusion list)
08:17:21.05 +52:15:09.2 -- not an asteroid (will add it to exclusion list)
08:16:24.41 +49:29:13.6 -- not an asteroid (will add it to exclusion list)
08:29:48.66 +56:04:33.4 -- not an asteroid (will add it to exclusion list)
08:26:50.11 +48:55:55.6 -- asteroid (will NOT add it to exclusion list)
07:34:44.72 +57:52:57.3 -- not an asteroid (will add it to exclusion list)
08:17:54.11 +50:08:08.5 -- not an asteroid (will add it to exclusion list)
08:59:43.33 +58:30:39.8 -- not an asteroid (will add it to exclusion list)
08:45:23.06 +55:11:44.6 -- not an asteroid (will add it to exclusion list)
07:34:44.80 +58:28:41.1 -- not an asteroid (will add it to exclusion list)
08:07:33.55 +49:02:17.8 -- not an asteroid (will add it to exclusion list)
07:52:49.62 +50:19:49.1 -- not an asteroid (will add it to exclusion list)
08:30:37.64 +51:06:21.3 -- not an asteroid (will add it to exclusion list)
08:38:01.66 +52:01:21.1 -- not an asteroid (will add it to exclusion list)
08:02:58.18 +53:38:06.6 -- not an asteroid (will add it to exclusion list)
08:13:01.44 +54:31:15.9 -- not an asteroid (will add it to exclusion list)
08:19:18.12 +55:55:20.4 -- not an asteroid (will add it to exclusion list)
08:21:42.68 +50:00:19.9 -- not an asteroid (will add it to exclusion list)
08:09:55.59 +55:33:44.5 -- not an asteroid (will add it to exclusion list)
08:17:42.83 +52:04:08.2 -- not an asteroid (will add it to exclusion list)
08:11:54.46 +53:41:57.4 -- not an asteroid (will add it to exclusion list)
08:20:13.67 +51:04:59.7 -- not an asteroid (will add it to exclusion list)
08:44:32.92 +55:38:03.2 -- not an asteroid (will add it to exclusion list)
08:17:46.23 +55:14:16.0 -- not an asteroid (will add it to exclusion list)
08:26:40.76 +52:16:14.3 -- not an asteroid (will add it to exclusion list)
08:43:33.11 +56:05:22.5 -- not an asteroid (will add it to exclusion list)
08:16:45.76 +51:28:12.0 -- not an asteroid (will add it to exclusion list)
08:32:27.42 +54:28:06.5 -- not an asteroid (will add it to exclusion list)
08:06:33.81 +54:30:34.0 -- not an asteroid (will add it to exclusion list)
07:53:14.38 +49:37:44.5 -- not an asteroid (will add it to exclusion list)
08:25:28.73 +52:13:37.8 -- not an asteroid (will add it to exclusion list)
08:08:36.56 +52:36:42.5 -- not an asteroid (will add it to exclusion list)
08:16:28.29 +49:57:20.4 -- not an asteroid (will add it to exclusion list)
08:48:00.70 +58:37:52.2 -- not an asteroid (will add it to exclusion list)
08:38:40.47 +55:51:14.8 -- not an asteroid (will add it to exclusion list)
08:12:02.65 +49:06:12.1 -- not an asteroid (will add it to exclusion list)
07:52:01.91 +53:28:17.2 -- not an asteroid (will add it to exclusion list)
08:16:50.27 +49:05:57.4 -- not an asteroid (will add it to exclusion list)
08:55:57.77 +54:37:03.4 -- not an asteroid (will add it to exclusion list)
08:07:40.69 +54:24:36.6 -- not an asteroid (will add it to exclusion list)
08:33:19.87 +52:03:06.8 -- not an asteroid (will add it to exclusion list)
08:16:47.27 +53:19:27.1 -- not an asteroid (will add it to exclusion list)
08:23:50.71 +49:51:51.7 -- not an asteroid (will add it to exclusion list)
08:04:39.72 +53:03:21.7 -- not an asteroid (will add it to exclusion list)
08:12:11.82 +52:10:51.4 -- not an asteroid (will add it to exclusion list)
08:06:32.76 +56:24:07.0 -- not an asteroid (will add it to exclusion list)
07:57:42.82 +52:17:01.7 -- not an asteroid (will add it to exclusion list)
08:17:41.87 +50:22:47.5 -- not an asteroid (will add it to exclusion list)
08:22:55.67 +54:34:22.5 -- not an asteroid (will add it to exclusion list)
08:39:14.67 +57:35:57.3 -- not an asteroid (will add it to exclusion list)
08:08:43.10 +55:33:31.6 -- not an asteroid (will add it to exclusion list)
07:47:52.93 +51:09:31.9 -- not an asteroid (will add it to exclusion list)
08:08:35.55 +51:53:33.5 -- not an asteroid (will add it to exclusion list)
07:51:48.53 +51:58:36.3 -- not an asteroid (will add it to exclusion list)
08:26:22.19 +54:32:23.8 -- not an asteroid (will add it to exclusion list)
08:10:40.42 +51:39:25.9 -- not an asteroid (will add it to exclusion list)
08:15:26.45 +52:32:07.1 -- not an asteroid (will add it to exclusion list)
08:06:23.34 +53:52:41.1 -- not an asteroid (will add it to exclusion list)
08:11:29.64 +52:51:13.0 -- not an asteroid (will add it to exclusion list)
07:52:58.50 +52:53:05.4 -- not an asteroid (will add it to exclusion list)
08:07:24.34 +50:18:18.2 -- not an asteroid (will add it to exclusion list)
07:54:25.44 +50:39:49.1 -- not an asteroid (will add it to exclusion list)
08:40:06.01 +49:52:55.7 -- not an asteroid (will add it to exclusion list)
08:09:20.71 +49:41:15.1 -- not an asteroid (will add it to exclusion list)
08:11:21.13 +52:44:23.5 -- not an asteroid (will add it to exclusion list)
08:24:24.41 +50:00:50.4 -- not an asteroid (will add it to exclusion list)
08:40:49.50 +50:08:14.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:31:05.44 +58:13:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:31:51.09 +57:58:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:11.36 +58:27:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:48.15 +56:59:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:32:49.55 +58:06:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:03.73 +57:22:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:26.27 +57:47:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:30.92 +56:35:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:33:35.43 +55:55:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:19.47 +58:09:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:42.45 +56:39:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:44.72 +57:52:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:44.80 +58:28:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:57.58 +56:29:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:04.51 +58:01:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:17.46 +58:24:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:30.82 +57:28:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:45.61 +58:16:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:54.59 +56:58:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:01.52 +56:32:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:11.73 +58:05:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:18.42 +57:09:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:02.08 +57:52:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:20.06 +57:39:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:35.15 +55:38:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:47.10 +56:47:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:54.68 +57:19:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:56.32 +58:12:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:33.22 +57:53:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:49.02 +58:29:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:34.93 +58:26:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:21.68 +58:41:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:52.93 +51:09:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:58.73 +51:44:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:48.53 +51:58:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:01.91 +53:28:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:49.62 +50:19:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:58.50 +52:53:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:14.38 +49:37:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:54:25.44 +50:39:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:56:16.97 +53:45:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:57:42.82 +52:17:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:58:10.51 +51:12:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:58:44.51 +57:15:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:00:48.23 +54:07:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:02:45.70 +52:44:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:02:58.18 +53:38:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:03:46.18 +57:19:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:31.04 +51:21:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:35.78 +56:21:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:39.72 +53:03:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:08.26 +49:02:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:23.34 +53:52:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:32.76 +56:24:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:33.81 +54:30:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:06:41.30 +53:24:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:24.34 +50:18:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:33.55 +49:02:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:40.69 +54:24:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:56.59 +55:02:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:08:35.55 +51:53:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:08:36.56 +52:36:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:08:43.10 +55:33:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:09:20.71 +49:41:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:09:55.59 +55:33:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:40.42 +51:39:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:21.13 +52:44:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:29.64 +52:51:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:50.52 +49:33:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:54.46 +53:41:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:02.65 +49:06:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:11.82 +52:10:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:01.44 +54:31:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:03.24 +49:24:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:07.93 +55:00:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:26.45 +52:32:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:03.36 +58:22:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:24.41 +49:29:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:28.29 +49:57:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:45.76 +51:28:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:47.27 +53:19:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:50.27 +49:05:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:21.05 +52:15:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:41.87 +50:22:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:42.83 +52:04:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:46.23 +55:14:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:54.11 +50:08:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:50.04 +56:16:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:18.12 +55:55:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:13.67 +51:04:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:42.68 +50:00:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:55.67 +54:34:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:50.71 +49:51:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:02.85 +58:57:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:24.41 +50:00:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:28.73 +52:13:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:22.19 +54:32:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:40.76 +52:16:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:05.31 +55:04:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:48.66 +56:04:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:37.64 +51:06:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:32:27.42 +54:28:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:33:19.87 +52:03:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:01.66 +52:01:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:40.47 +55:51:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:39:14.67 +57:35:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:06.01 +49:52:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:49.50 +50:08:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:43:33.11 +56:05:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:44:32.92 +55:38:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:45:23.06 +55:11:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:00.70 +58:37:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:55:57.77 +54:37:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:59:43.33 +58:30:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:28.33 +52:41:21.2 -- 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)
07:31:05.44 +58:13:05.1 -- not a known variable star
07:31:51.09 +57:58:09.5 -- not a known variable star
07:32:11.36 +58:27:05.4 -- not a known variable star
07:32:48.15 +56:59:29.8 -- not a known variable star
07:32:49.55 +58:06:03.7 -- a known variable star
07:33:03.73 +57:22:33.4 -- not a known variable star
07:33:26.27 +57:47:50.2 -- not a known variable star
07:33:30.92 +56:35:02.6 -- not a known variable star
07:33:35.43 +55:55:45.6 -- not a known variable star
07:34:19.47 +58:09:21.4 -- not a known variable star
07:34:42.45 +56:39:57.9 -- not a known variable star
07:34:44.72 +57:52:57.3 -- not a known variable star
07:34:44.80 +58:28:41.1 -- not a known variable star
07:34:57.58 +56:29:31.9 -- not a known variable star
07:35:04.51 +58:01:16.1 -- not a known variable star
07:35:17.46 +58:24:10.8 -- not a known variable star
07:35:30.82 +57:28:50.8 -- not a known variable star
07:35:45.61 +58:16:49.4 -- not a known variable star
07:35:54.59 +56:58:53.8 -- not a known variable star
07:36:01.52 +56:32:38.1 -- not a known variable star
07:36:11.73 +58:05:21.6 -- not a known variable star
07:36:18.42 +57:09:53.8 -- not a known variable star
07:37:02.08 +57:52:50.9 -- not a known variable star
07:37:20.06 +57:39:30.5 -- not a known variable star
07:37:35.15 +55:38:53.4 -- not a known variable star
07:37:47.10 +56:47:51.1 -- not a known variable star
07:37:54.68 +57:19:53.7 -- not a known variable star
07:37:56.32 +58:12:07.0 -- not a known variable star
07:39:33.22 +57:53:54.5 -- not a known variable star
07:39:49.02 +58:29:22.2 -- not a known variable star
07:40:34.93 +58:26:28.0 -- not a known variable star
07:44:21.68 +58:41:28.8 -- not a known variable star
07:47:52.93 +51:09:31.9 -- not a known variable star
07:49:58.73 +51:44:41.7 -- not a known variable star
07:51:48.53 +51:58:36.3 -- not a known variable star
07:52:01.91 +53:28:17.2 -- not a known variable star
07:52:49.62 +50:19:49.1 -- not a known variable star
07:52:58.50 +52:53:05.4 -- not a known variable star
07:53:14.38 +49:37:44.5 -- not a known variable star
07:54:25.44 +50:39:49.1 -- not a known variable star
07:56:16.97 +53:45:57.2 -- not a known variable star
07:57:42.82 +52:17:01.7 -- not a known variable star
07:58:10.51 +51:12:03.6 -- not a known variable star
07:58:44.51 +57:15:32.9 -- not a known variable star
08:00:48.23 +54:07:56.4 -- not a known variable star
08:02:45.70 +52:44:30.0 -- not a known variable star
08:02:58.18 +53:38:06.6 -- not a known variable star
08:03:46.18 +57:19:10.9 -- not a known variable star
08:04:31.04 +51:21:15.9 -- not a known variable star
08:04:35.78 +56:21:35.4 -- a known variable star
08:04:39.72 +53:03:21.7 -- not a known variable star
08:06:08.26 +49:02:14.8 -- not a known variable star
08:06:23.34 +53:52:41.1 -- not a known variable star
08:06:32.76 +56:24:07.0 -- not a known variable star
08:06:33.81 +54:30:34.0 -- not a known variable star
08:06:41.30 +53:24:12.5 -- not a known variable star
08:07:24.34 +50:18:18.2 -- not a known variable star
08:07:33.55 +49:02:17.8 -- not a known variable star
08:07:40.69 +54:24:36.6 -- not a known variable star
08:07:56.59 +55:02:27.2 -- not a known variable star
08:08:35.55 +51:53:33.5 -- not a known variable star
08:08:36.56 +52:36:42.5 -- not a known variable star
08:08:43.10 +55:33:31.6 -- not a known variable star
08:09:20.71 +49:41:15.1 -- not a known variable star
08:09:55.59 +55:33:44.5 -- not a known variable star
08:10:40.42 +51:39:25.9 -- not a known variable star
08:11:21.13 +52:44:23.5 -- not a known variable star
08:11:29.64 +52:51:13.0 -- a known variable star
08:11:50.52 +49:33:53.3 -- not a known variable star
08:11:54.46 +53:41:57.4 -- not a known variable star
08:12:02.65 +49:06:12.1 -- not a known variable star
08:12:11.82 +52:10:51.4 -- not a known variable star
08:13:01.44 +54:31:15.9 -- not a known variable star
08:14:03.24 +49:24:37.9 -- not a known variable star
08:15:07.93 +55:00:04.7 -- not a known variable star
08:15:26.45 +52:32:07.1 -- not a known variable star
08:16:03.36 +58:22:27.0 -- not a known variable star
08:16:24.41 +49:29:13.6 -- a known variable star
08:16:28.29 +49:57:20.4 -- not a known variable star
08:16:45.76 +51:28:12.0 -- not a known variable star
08:16:47.27 +53:19:27.1 -- not a known variable star
08:16:50.27 +49:05:57.4 -- not a known variable star
08:17:21.05 +52:15:09.2 -- not a known variable star
08:17:41.87 +50:22:47.5 -- not a known variable star
08:17:42.83 +52:04:08.2 -- not a known variable star
08:17:46.23 +55:14:16.0 -- not a known variable star
08:17:54.11 +50:08:08.5 -- not a known variable star
08:18:50.04 +56:16:22.1 -- not a known variable star
08:19:18.12 +55:55:20.4 -- not a known variable star
08:20:13.67 +51:04:59.7 -- not a known variable star
08:21:42.68 +50:00:19.9 -- not a known variable star
08:22:55.67 +54:34:22.5 -- not a known variable star
08:23:50.71 +49:51:51.7 -- not a known variable star
08:24:02.85 +58:57:22.6 -- not a known variable star
08:24:24.41 +50:00:50.4 -- a known variable star
08:25:28.73 +52:13:37.8 -- not a known variable star
08:26:22.19 +54:32:23.8 -- not a known variable star
08:26:40.76 +52:16:14.3 -- not a known variable star
08:29:05.31 +55:04:05.3 -- not a known variable star
08:29:48.66 +56:04:33.4 -- not a known variable star
08:30:37.64 +51:06:21.3 -- not a known variable star
08:32:27.42 +54:28:06.5 -- not a known variable star
08:33:19.87 +52:03:06.8 -- not a known variable star
08:38:01.66 +52:01:21.1 -- not a known variable star
08:38:40.47 +55:51:14.8 -- not a known variable star
08:39:14.67 +57:35:57.3 -- not a known variable star
08:40:06.01 +49:52:55.7 -- not a known variable star
08:40:49.50 +50:08:14.2 -- a known variable star
08:43:33.11 +56:05:22.5 -- not a known variable star
08:44:32.92 +55:38:03.2 -- a known variable star
08:45:23.06 +55:11:44.6 -- a known variable star
08:48:00.70 +58:37:52.2 -- not a known variable star
08:55:57.77 +54:37:03.4 -- not a known variable star
08:59:43.33 +58:30:39.8 -- not a known variable star
09:10:28.33 +52:41:21.2 -- a known variable star
Found 106 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
115 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.77105466 -observatory 500
23:23:38.41 -01:55:50.2 Mercury (-0.1mag)
23:04:56.57 -07:26:47.6 Venus (-3.9mag)
21:43:07.80 -14:51:14.6 Mars (1.1mag)
07:06:04.56 +22:54:22.8 Jupiter (-2.5mag)
00:05:28.79 -01:44:10.6 Saturn (1.0mag)
03:39:59.90 +19:21:45.2 Uranus (5.7mag)
00:03:41.67 -01:01:32.2 Neptune (7.8mag)
20:29:07.81 -22:59:32.4 Pluto (14.5mag)
01:59:48.29 +16:49:53.5 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 03:26 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.77105466:
07:06:11.28 +22:54:11.4 Io (5.4mag)
07:06:17.40 +22:53:58.3 Europa (5.5mag)
07:05:57.56 +22:54:44.4 Ganymede (4.9mag)
07:06:25.12 +22:53:54.2 Callisto (6.2mag)
07:09:13.99 +23:10:42.7 Himalia (15.0mag)
07:06:08.45 +22:54:15.8 Thebe (15.9mag)
07:08:38.99 +23:19:15.3 Elara (17.0mag)
07:01:38.44 +24:02:17.6 Pasiphae (17.0mag)
07:15:05.43 +22:42:24.7 Carme (18.1mag)
00:05:40.59 -01:44:14.8 Titan (8.8mag)
00:05:34.47 -01:44:08.9 Rhea (10.1mag)
00:05:24.46 -01:45:30.9 Iapetus (11.5mag)
00:05:30.05 -01:44:14.0 Hyperion (14.8mag)
00:07:33.05 -01:31:10.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 03:26 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.77105466:
08:46:41.36 +24:30:48.9 JWST
13:38:53.39 +54:19:45.7 Chandra
16:40:10.83 -50:14:06.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 03:26 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)2461093.77105466 at 500
16:59:55.15 -11:03:54.7 17.5mag 10P/Tempel 2
03:37:25.50 +28:58:13.6 18.0mag 123P/West-Hartley
08:23:27.78 +60:40:46.8 18.4mag 124P/Mrkos
21:19:57.79 -07:36:50.2 22.1mag 141P/Machholz
01:21:24.45 +11:56:49.4 17.7mag 145P/Shoemaker-Levy 5
11:02:52.36 +30:35:19.3 17.9mag 164P/Christensen
09:33:04.07 -33:51:29.6 18.0mag 195P/Hill
15:52:02.48 -06:35:13.1 19.2mag 210P/Christensen
18:17:23.95 -21:28:06.3 17.3mag 218P/LINEAR
04:45:22.45 +19:21:16.8 0.0mag 235P/LINEAR
03:56:33.36 +27:45:47.5 17.8mag 240P/NEAT
15:17:46.06 +06:37:53.7 14.8mag 24P/Schaumasse
11:23:28.24 -03:22:58.8 17.4mag 29P/Schwassmann-Wachmann 1
07:03:46.99 +27:24:52.3 19.6mag 407P/PanSTARRS-Fuls
17:07:20.35 -11:19:11.0 17.6mag 40P/Vaisala 1
11:02:08.31 -08:51:29.1 16.6mag 43P/Wolf-Harrington
13:25:30.15 -05:50:01.4 20.0mag 489P/Denning
04:34:27.36 +48:33:59.7 17.8mag 493P/2024 Q2 (LONEOS)
06:04:25.96 +47:30:09.6 17.7mag 63P/Wild 1
23:14:50.47 -02:06:13.6 16.2mag 78P/Gehrels 2
20:01:56.55 -22:17:16.6 14.9mag 88P/Howell
15:27:58.16 -29:01:14.4 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.80 -72:35:30.0 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:48.96 +31:12:55.3 18.2mag C/2017 K2 (PanSTARRS)
20:06:42.15 -65:11:51.4 18.1mag C/2020 V2 (ZTF)
17:21:43.38 +04:22:07.3 16.3mag C/2021 G2 (ATLAS)
03:35:46.65 +24:36:50.8 15.8mag C/2022 N2 (PanSTARRS)
09:08:10.81 +29:50:08.8 15.3mag C/2022 QE78 (ATLAS)
08:35:38.41 -06:32:54.8 16.7mag C/2022 R6 (PanSTARRS)
23:53:11.06 +48:27:02.9 18.0mag C/2023 C2 (ATLAS)
09:51:00.03 -20:44:57.4 17.5mag C/2023 F3 (ATLAS)
20:34:59.44 +61:14:31.4 17.3mag C/2023 H5 (Lemmon)
19:34:30.95 -03:24:19.4 16.1mag C/2023 R1 (PANSTARRS)
02:48:57.69 +35:40:31.0 18.5mag C/2023 RS61 (PanSTARRS)
21:01:38.92 +81:20:05.6 18.0mag C/2023 X2 (Lemmon)
06:38:59.45 +63:49:23.2 17.3mag C/2024 A1 (ATLAS)
01:57:37.33 -24:28:04.8 11.2mag C/2024 E1 (Wierzchos)
11:44:53.09 -02:33:30.4 18.1mag C/2024 G2 (ATLAS)
19:28:25.80 +00:39:27.0 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.51 -01:41:57.3 17.7mag C/2024 G6 (ATLAS)
19:53:32.48 +03:16:25.0 15.6mag C/2024 J3 (ATLAS)
02:47:18.38 -31:33:08.1 15.4mag C/2024 T5 (ATLAS)
16:24:46.63 -58:16:33.8 15.6mag C/2025 A6 (Lemmon)
04:50:28.12 +62:11:42.0 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)
15:56:38.49 -12:55:22.4 14.8mag C/2025 L1 (ATLAS)
02:20:20.14 -19:06:58.0 16.7mag C/2025 Q3 (ATLAS)
02:09:43.59 +17:17:24.7 21.2mag C/2025 R2 (SWAN)
22:20:48.43 +17:39:25.0 16.4mag C/2025 R3 (PANSTARRS)
21:46:08.80 -16:51:55.8 21.5mag C/2025 T1 (ATLAS)
03:05:58.16 -20:30:34.9 18.3mag C/2026 A1 (MAPS)
21:03:28.59 +20:58:50.6 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 03:27 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 22 03:26 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 22 03:26 tocp_transients_list.txt