This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0719 Cyg,2461126.9403,11.05,0.05,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
V0719 Cyg 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:39.70 +30:28:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194702.60+283753.3,2461126.9403,11.84,0.05,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
ZTF J194702.60+283753.3 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:01.73 +28:37:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2032150792469213696,2461126.9403,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2032150792469213696 20260327.4403 11.85CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:19.02 +30:34:12.7 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028529413473516800,2461126.9403,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028529413473516800 20260327.4403 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:41.81 +28:32:36.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055275514828580352,2461126.9403,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2055275514828580352 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:08:42.76 +33:33:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:26.50 +32:07:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055275514828580352,2461126.9403,13.52,0.05,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 2055275514828580352 20260327.4403 13.52CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:08:43.59 +33:33:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.31 20:13:59.19 +26:26:08.2
65.73591 -4.46645 galactic Vul Second-epoch detections are separated by 4.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1835712143787421696 | 20:13:59.24 +26:25:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M4 (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 1835712143787421696,2461126.9403,13.31,0.05,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
Gaia DR3 1835712143787421696 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:59.19 +26:26:08.2 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.13 19:37:25.75 +33:58:20.5
68.10479 6.18159 galactic Cyg Second-epoch detections are separated by 0.7" 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 | ATO J294.3506+33.9766 | 19:37:25.75 +33:58:20.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J294.3506+33.9766,2461126.9403,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.3506+33.9766 20260327.4403 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:25.75 +33:58:20.5 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.18 19:48:09.87 +33:49:37.5
69.07549 4.16948 galactic Cyg Second-epoch detections are separated by 4.4" 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 J297.0387+33.8288 | 19:48:09.87 +33:49:37.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J297.0387+33.8288,2461126.9403,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.0387+33.8288 20260327.4403 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:09.87 +33:49:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195734.79+325730.3,2461126.9403,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195734.79+325730.3 20260327.4403 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:33.61 +32:57:34.9 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.05 19:31:37.14 +29:52:29.9
63.89491 5.30867 galactic Cyg Second-epoch detections are separated by 5.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.9057+29.8791 | 19:31:37.14 +29:52:29.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J292.9057+29.8791,2461126.9403,13.05,0.05,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 J292.9057+29.8791 20260327.4403 13.05CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:37.14 +29:52:29.9 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.18 19:56:49.79 +33:00:47.9
69.29898 2.19931 galactic Cyg Second-epoch detections are separated by 5.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.2105+33.0176 | 19:56:50.83 +33:00:49.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.2105+33.0176,2461126.9403,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2105+33.0176 20260327.4403 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:49.79 +33:00:47.9 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.91 19:31:03.49 +34:06:32.8
67.59647 7.40871 galactic Cyg Second-epoch detections are separated by 7.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.7541+34.1102 | 19:31:03.49 +34:06:32.8 (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 J292.7541+34.1102,2461126.9403,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.7541+34.1102 20260327.4403 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:03.49 +34:06:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026088806864357760,2461126.9403,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026088806864357760 20260327.4403 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:30.30 +27:46:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:08.28 +34:14:49.7 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194324.39+331322.5,2461126.9403,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194324.39+331322.5 20260327.4403 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:24.07 +33:13:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.06 19:48:28.45 +31:50:33.0
67.38913 3.11565 galactic Cyg Second-epoch detections are separated by 5.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.1165+31.8410 | 19:48:28.45 +31:50:33.0 (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 J297.1165+31.8410,2461126.9403,13.06,0.05,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 J297.1165+31.8410 20260327.4403 13.06CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:28.45 +31:50:33.0 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200117.73+333730.0,2461126.9403,13.05,0.05,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
ZTF J200117.73+333730.0 20260327.4403 13.05CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:17.47 +33:37:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1860091344540716544,2461126.9403,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1860091344540716544 20260327.4403 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:47.02 +28:12:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2046930874428984448,2461126.9403,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046930874428984448 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:28.67 +33:25:16.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.05 19:54:08.89 +31:39:43.9
67.84863 1.98574 galactic Cyg Second-epoch detections are separated by 6.2" 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 | ATO J298.5352+31.6627 | 19:54:08.89 +31:39:43.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J298.5352+31.6627,2461126.9403,13.05,0.05,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 J298.5352+31.6627 20260327.4403 13.05CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:08.89 +31:39:43.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194154.38+291233.8,2461126.9403,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194154.38+291233.8 20260327.4403 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:53.57 +29:12:34.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:16.49 +33:50:54.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194826.74+305325.0,2461126.9403,13.05,0.05,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
ZTF J194826.74+305325.0 20260327.4403 13.05CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:27.17 +30:53:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.77 19:45:21.72 +34:09:05.0
69.06697 4.83473 galactic Cyg Second-epoch detections are separated by 2.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.3330+34.1415 | 19:45:21.72 +34:09:05.0 (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 J296.3330+34.1415,2461126.9403,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.3330+34.1415 20260327.4403 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:21.72 +34:09:05.0 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.00 19:51:18.82 +31:56:40.9
67.78298 2.64770 galactic Cyg Second-epoch detections are separated by 2.5" 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 J297.8319+31.9495 | 19:51:18.82 +31:56:40.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J297.8319+31.9495,2461126.9403,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.8319+31.9495 20260327.4403 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:18.82 +31:56:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.82 19:43:07.55 +33:23:29.2
68.17348 4.86357 galactic Cyg 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 | ATO J295.7811+33.3900 | 19:43:07.55 +33:23:29.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J295.7811+33.3900,2461126.9403,12.82,0.05,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
ATO J295.7811+33.3900 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:07.55 +33:23:29.2 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.81 19:39:52.24 +31:14:35.2
65.95654 4.41021 galactic Cyg Second-epoch detections are separated by 3.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.9672+31.2470 | 19:39:52.24 +31:14:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J294.9672+31.2470,2461126.9403,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.9672+31.2470 20260327.4403 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:52.24 +31:14:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.61 19:32:27.33 +33:10:15.7
66.89943 6.71153 galactic Cyg Second-epoch detections are separated by 7.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.1171+33.1699 | 19:32:27.33 +33:10:15.7 (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 J293.1171+33.1699,2461126.9403,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.1171+33.1699 20260327.4403 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:27.33 +33:10:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030047594181363712,2461126.9403,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030047594181363712 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:55.25 +29:20:05.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195045.89+324045.3,2461126.9403,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195045.89+324045.3 20260327.4403 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:45.43 +32:40:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.56 19:46:01.52 +33:42:32.4
68.75023 4.49565 galactic Cyg Second-epoch detections are separated by 8.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.5123+33.7107 | 19:46:01.52 +33:42:32.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.310+/-0.054 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.5123+33.7107,2461126.9403,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.5123+33.7107 20260327.4403 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:01.52 +33:42:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035051441581305472,2461126.9403,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035051441581305472 20260327.4403 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:58.26 +33:50:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.69 19:37:50.22 +32:17:10.0
66.66088 5.29461 galactic Cyg 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 | ATO J294.4705+32.2992 | 19:37:53.02 +32:17:40.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J294.4705+32.2992,2461126.9403,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.4705+32.2992 20260327.4403 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:50.22 +32:17:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:52.38 +32:38:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2033234601684879744,2461126.9403,12.63,0.05,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 2033234601684879744 20260327.4403 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:17.29 +31:25:36.6 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.55 19:34:11.64 +31:30:50.1
65.60750 5.60202 galactic Cyg 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 | ATO J293.5479+31.5042 | 19:34:09.76 +31:30:47.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1950ApJ...112...90M LF 2 +31 53
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J293.5479+31.5042,2461126.9403,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.5479+31.5042 20260327.4403 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:34:11.64 +31:30:50.1 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2045077681932415744,2461126.9403,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2045077681932415744 20260327.4403 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:20.61 +31:43:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.98 19:42:46.51 +32:37:26.4
67.46683 4.54991 galactic Cyg Second-epoch detections are separated by 2.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.6900+32.6363 | 19:42:47.64 +32:37:54.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A4II 1960LS....C02....0S LS II +32 3
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J295.6900+32.6363,2461126.9403,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.6900+32.6363 20260327.4403 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:46.51 +32:37:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.53 19:43:14.55 +31:40:57.8
66.69456 3.99972 galactic Cyg Second-epoch detections are separated by 1.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.8067+31.6936 | 19:43:13.63 +31:41:37.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.8067+31.6936,2461126.9403,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.8067+31.6936 20260327.4403 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:14.55 +31:40:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.55 19:40:08.55 +26:19:50.0
61.69761 1.94914 galactic Vul 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 | ATO J295.0349+26.3244 | 19:40:08.37 +26:19:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J295.0349+26.3244,2461126.9403,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.0349+26.3244 20260327.4403 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:08.55 +26:19:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.03 19:54:40.86 +28:47:20.5
65.44560 0.40565 galactic Vul Second-epoch detections are separated by 4.7" 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 | Large-amplitude variable Gaia DR2 2028537075673664000 | 19:54:41.47 +28:46:35.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2028537075673664000,2461126.9403,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2028537075673664000 20260327.4403 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:40.86 +28:47:20.5 ;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_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.81 19:50:25.38 +30:34:07.2
66.50032 2.11167 galactic Cyg Second-epoch detections are separated by 4.1" 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 | ATO J297.6138+30.5690 | 19:50:25.38 +30:34:07.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J297.6138+30.5690,2461126.9403,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.6138+30.5690 20260327.4403 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:25.38 +30:34:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.26 19:36:38.06 +31:30:02.9
65.84649 5.13931 galactic Cyg Second-epoch detections are separated by 2.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.1568+31.4986 | 19:36:38.06 +31:30:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J294.1568+31.4986,2461126.9403,12.26,0.05,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
ATO J294.1568+31.4986 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:38.06 +31:30:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030480703028656896,2461126.9403,13.54,0.05,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 2030480703028656896 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:38.16 +30:48:00.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 12333,2461126.9403,13.06,0.05,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
NSV 12333 20260327.4403 13.06CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:35.05 +28:56:19.4 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.35 19:37:40.95 +31:17:34.0
65.77206 4.84298 galactic Cyg Second-epoch detections are separated by 0.9" 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 | ATO J294.4221+31.2912 | 19:37:40.95 +31:17:34.0 (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 J294.4221+31.2912,2461126.9403,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.4221+31.2912 20260327.4403 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:40.95 +31:17:34.0 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.76 19:28:41.35 +31:44:00.8
65.24586 6.73877 galactic Cyg Second-epoch detections are separated by 4.0" 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 | ATO J292.1579+31.7343 | 19:28:39.32 +31:44:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.1579+31.7343,2461126.9403,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.1579+31.7343 20260327.4403 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:41.35 +31:44:00.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:30.82 +29:36:28.6 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.49 20:10:05.70 +27:04:39.4
65.79900 -3.38810 galactic Vul Second-epoch detections are separated by 1.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J302.5214+27.0771 | 20:10:05.70 +27:04:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J302.5214+27.0771,2461126.9403,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.5214+27.0771 20260327.4403 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:05.70 +27:04:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195130.35+313134.4,2461126.9403,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195130.35+313134.4 20260327.4403 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:30.22 +31:31:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194533.10+282118.1,2461126.9403,11.85,0.05,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
ZTF J194533.10+282118.1 20260327.4403 11.85CV 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:33.66 +28:21:29.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1835024128706633856,2461126.9403,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835024128706633856 20260327.4403 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:06.37 +25:52:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2024570931113624320,2461126.9403,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2024570931113624320 20260327.4403 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:34:27.78 +26:01:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:55.65 +33:29:48.7 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.39 19:39:53.07 +28:15:05.5
63.34389 2.94321 galactic Cyg 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 | ATO J294.9717+28.2485 | 19:39:53.07 +28:15:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J294.9717+28.2485,2461126.9403,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.9717+28.2485 20260327.4403 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:53.07 +28:15:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.76 19:32:14.14 +31:41:33.2
65.56624 6.05379 galactic Cyg Second-epoch detections are separated by 4.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2044901412156526208 | 19:32:17.01 +31:41:50.3 (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 2044901412156526208,2461126.9403,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2044901412156526208 20260327.4403 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:14.14 +31:41:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.73 20:02:44.55 +31:47:01.8
68.90818 0.49153 galactic Cyg Second-epoch detections are separated by 4.7" 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 J300.6970+31.7865 | 20:02:45.40 +31:47:10.4 (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 J300.6970+31.7865,2461126.9403,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.6970+31.7865 20260327.4403 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:44.55 +31:47:01.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.98 19:31:13.45 +27:49:32.6
62.04450 4.41004 galactic Cyg Second-epoch detections are separated by 4.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.8168+27.8294 | 19:31:13.45 +27:49:32.6 (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 J292.8168+27.8294,2461126.9403,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.8168+27.8294 20260327.4403 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:13.45 +27:49:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.62 19:29:48.75 +27:27:14.7
61.56746 4.50839 galactic Vul 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 | 19:29:48.75 +27:27:14.7 (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,2461126.9403,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:48.75 +27:27:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030322987489376256,2461126.9403,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030322987489376256 20260327.4403 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:26.16 +29:50:23.6 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2032185701966162688,2461126.9403,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2032185701966162688 20260327.4403 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:33.78 +30:33:16.1 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.66 19:35:17.38 +25:42:29.2
60.62109 2.59642 galactic Vul 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 | ATO J293.8301+25.7048 | 19:35:17.38 +25:42:29.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J293.8301+25.7048,2461126.9403,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.8301+25.7048 20260327.4403 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:17.38 +25:42:29.2 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.35 20:00:05.84 +30:07:46.0
67.20407 0.09825 galactic Cyg Second-epoch detections are separated by 3.4" 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 | ATO J300.0316+30.1282 | 20:00:05.31 +30:07:39.4 (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 J300.0316+30.1282,2461126.9403,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0316+30.1282 20260327.4403 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:00:05.84 +30:07:46.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.9403,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4403 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:51.22 +26:56:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.47 19:27:15.07 +33:36:39.8
66.78131 7.87770 galactic Cyg Second-epoch detections are separated by 3.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2046605453323851392 | 19:27:14.01 +33:36:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2046605453323851392,2461126.9403,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046605453323851392 20260327.4403 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:27:15.07 +33:36:39.8 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.79 19:31:55.29 +31:33:45.0
65.41920 6.05116 galactic Cyg Second-epoch detections are separated by 4.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.9802+31.5640 | 19:31:55.29 +31:33:45.0 (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 J292.9802+31.5640,2461126.9403,12.79,0.05,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
ATO J292.9802+31.5640 20260327.4403 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:55.29 +31:33:45.0 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J1947370+264540,2461126.9403,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1947370+264540 20260327.4403 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:36.69 +26:45:43.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2046951043596611072,2461126.9403,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2046951043596611072 20260327.4403 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:55.92 +33:40:49.7 ;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_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 11.95 19:34:48.00 +33:15:46.2
67.21464 6.32320 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.7061+33.2588 | 19:34:47.75 +33:15:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.7061+33.2588,2461126.9403,11.95,0.05,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
ATO J293.7061+33.2588 20260327.4403 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:34:48.00 +33:15:46.2 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2032422612361636224,2461126.9403,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2032422612361636224 20260327.4403 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:04.23 +29:51:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 12.94 19:33:10.71 +30:07:50.3
64.28206 5.13342 galactic Cyg Second-epoch detections are separated by 4.3" 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 | ATO J293.2942+30.1307 | 19:33:10.71 +30:07:50.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.258+/-0.145 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.2942+30.1307,2461126.9403,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2942+30.1307 20260327.4403 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:10.71 +30:07:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4403 2461126.9403 13.37 19:47:53.64 +32:03:00.1
67.50675 3.32642 galactic Cyg Second-epoch detections are separated by 4.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.9719+32.0498 | 19:47:53.64 +32:03:00.1 (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 J296.9719+32.0498,2461126.9403,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.9719+32.0498 20260327.4403 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:53.64 +32:03:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20_00sec_-15_00C_LIGHT_0489_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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461126.94059248 27.03.2026 10:34:17.190 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 9 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): 26367
Objects passed selection criteria: 26344
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 24586.2
Average stars matched: 23845.5 (96.9871 %)
Memory usage VmPeak: 130452 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:19:59 CDT 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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461126.94059248 27.03.2026 10:34:17.190 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 275
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 92 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): 231795
Objects passed selection criteria: 231196
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 182840
Average stars matched: 175811 (96.1554 %)
Memory usage VmPeak: 2910400 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:26:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.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: 2461126.94004984
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:59.548 +30:01:06.34
Angular distance between the image centers 0.01 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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:58.179 +30:00:41.14
Angular distance between the image centers 0.01 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 19:59:59.548 +30:01:06.34
Second-epoch second image center 19:59:58.179 +30:00:41.14
Angular distance between the image centers 0.00857 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.qdnuX9V37L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.rKiuAD76HA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits &> /tmp/tmp.Ho24Hm7M0n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits &> /tmp/tmp.WSBUzyIHrV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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 7455 out of 30878 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854269
a=0.000000 b=1.000000 c=22.854269
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
4.1 pix fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
3.7 pix fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Limiting magnitude estimates:
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
14.3 mag. fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
14.4 mag. fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qdnuX9V37L (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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3756, passed=30878
Got 30878 stars (including 27089 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 30878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.90"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.54"
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 745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.51"
Estimated accuracy of the plate solution: 2.18"
Excluding outliers - 698 stars left (next iteration limit 694)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.rKiuAD76HA (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/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3771, passed=30931
Got 30931 stars (including 27121 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 30931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.95"
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 654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.91"
Estimated accuracy of the plate solution: 3.33"
Excluding outliers - 583 stars left (next iteration limit 586)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.Ho24Hm7M0n (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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1719, passed=24532
Got 24532 stars (including 22806 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat
util/solve_plate_with_UCAC5 got 24532 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 921 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.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.WSBUzyIHrV (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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2000, passed=26116
Got 26116 stars (including 24108 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat
util/solve_plate_with_UCAC5 got 26116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 933 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 920 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.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
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits'
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52478.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 2s
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Considering the candidate 52087_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52087_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 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 52090_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 52090_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 52391_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52391_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:58:56.67 +29:22:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52392_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52392_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:59:46.28 +29:15:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52395_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52395_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:02:05.37 +31:50:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52403_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52403_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:01.37 +28:47:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.065 2028701555785889920 297.25474329268 +28.79901216728 11.7517 11.2450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52427_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52427_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:56:15.88 +31:01:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52430_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52430_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:03:12.77 +32:53:02.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)
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Considering the candidate 52440_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52440_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:49.23 +30:16:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52456_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 52456_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 52462_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52462_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:47:24.20 +29:00:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52464_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52464_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:07.71 +28:19:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.393 2028435989353266432 298.03156911551 +28.33082786052 11.6876 11.1894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52465_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52465_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:58:57.32 +29:56:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52466_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52466_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52472_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52472_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:59:00.21 +28:32:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52474_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52474_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:34:30.49 +27:34:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52478_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 52478_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 52479_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52479_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:53.64 +28:53:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52481_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52481_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:56:51.27 +28:03:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52482_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52482_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:57:47.97 +30:33:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52488_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52488_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:57:14.69 +33:34:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.574 2034447363021206528 299.31173281795 +33.58106498367 11.9517 11.5631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52493_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52493_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:00:27.42 +26:10:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52495_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52495_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:41:44.79 +27:37:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52496_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52496_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:57:09.54 +29:00:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52498_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52498_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:54:18.58 +27:39:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.402 2027593660340304128 298.57716348573 +27.66067962414 12.1568 11.5671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52502_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52502_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:00:04.91 +26:41:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52508_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52508_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:47:11.45 +28:50:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52511_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52511_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:29.01 +25:47:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52517_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52517_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:55:30.54 +30:03:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52518_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52518_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:01:29.99 +30:17:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 5.750 2030254233642628224 300.37454698461 +30.29358164899 11.9865 11.3861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52519_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52519_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:51:22.12 +28:27:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 4.562 2028628781853779584 297.84078997297 +28.45795839704 11.8255 10.9264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52521_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52521_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:55:30.86 +29:12:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52524_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52524_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:50:21.29 +29:59:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52525_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52525_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:59:56.62 +29:44:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52526_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52526_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:49.98 +29:56:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.833 2032049358176941824 295.95789421681 +29.94728924820 11.8865 11.5312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52528_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52528_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:36:26.83 +29:58:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 3.912 2032479924410144512 294.11063361954 +29.96758216118 11.8805 11.3881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52530_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52530_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:55:02.15 +29:09:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.998 2028586686828712064 298.75841667345 +29.15687630648 11.8109 11.4859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52533_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52533_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:50:52.21 +29:09:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52536_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52536_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:56:35.28 +27:48:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52537_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52537_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:53.76 +29:37:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52539_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52539_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:54:30.82 +30:27:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 2.065 2030410673531735168 298.62775438253 +30.45902688354 11.8932 11.4132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52540_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52540_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:42.84 +27:26:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52541_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52541_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:05:46.38 +31:36:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.958 2030824747053134592 301.44274497704 +31.60725063988 11.8095 11.4103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52542_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52542_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:06:05.09 +28:51:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.872 2029124313646391552 301.52057007387 +28.85268081414 11.8415 11.4327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52543_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52543_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:54.78 +30:37:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52544_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52544_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:26.28 +28:26:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52545_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52545_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:29:00.28 +27:35:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.184 2026079323609382784 292.25054736578 +27.59521365732 11.8056 10.9881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52548_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52548_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:22.16 +28:32:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52549_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52549_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:57:07.26 +30:25:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.904 2030445312495031040 299.27966618226 +30.42167538830 11.8150 11.2885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52551_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52551_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:58:31.99 +30:20:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52552_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52552_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:39:36.01 +29:01:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52557_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52557_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:02:40.22 +29:07:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52562_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52562_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:51:36.87 +29:48:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52580_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 52580_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:10.50 +26:47:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09276_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 09276_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:33:52.24 +28:19:46.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Cyg-08-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 ####
20:03:39.70 +30:28:01.5
19:47:01.73 +28:37:58.4
19:48:19.02 +30:34:12.7
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:59.548 +30:01:06.34
Angular distance between the image centers 0.01 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 20:00:00.965 +30:00:24.17
Second-epoch image center 19:59:58.179 +30:00:41.14
Angular distance between the image centers 0.01 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 19:59:59.548 +30:01:06.34
Second-epoch second image center 19:59:58.179 +30:00:41.14
Angular distance between the image centers 0.00857 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.v79fjLGtDh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.I1Eqw5hZUs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits &> /tmp/tmp.33phd8ByNi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits &> /tmp/tmp.UvpxqDUkFk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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 8842 out of 281578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629178
a=0.000000 b=1.000000 c=22.629178
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 152 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
4.2 pix fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
3.8 pix fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Limiting magnitude estimates:
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
14.3 mag. fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
14.4 mag. fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.v79fjLGtDh (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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=51531, passed=281520
Got 281520 stars (including 229582 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 281520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.01"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.27"
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 754 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.27"
Estimated accuracy of the plate solution: 1.36"
Excluding outliers - 713 stars left (next iteration limit 698)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.I1Eqw5hZUs (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/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=51082, passed=280646
Got 280646 stars (including 229187 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 280646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 584 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: 3.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 4.22"
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 567 stars left (next iteration limit 568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.33phd8ByNi (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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=20156, passed=118386
Got 118386 stars (including 98174 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat
util/solve_plate_with_UCAC5 got 118386 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 934 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.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.UvpxqDUkFk (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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.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_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=23097, passed=133178
Got 133178 stars (including 109991 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat
util/solve_plate_with_UCAC5 got 133178 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 937 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.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
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-33-30_20.00sec_-15.00C_LIGHT_0489.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-08-Q2b1x1_071542_TTUQ2b1x1_6796_VIWf8Frm/wcs_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490.fits
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out125090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out221725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out275068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out316868.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out102097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out180042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out180224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out278809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83294.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 81s
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: 44s
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Considering the candidate 316815_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316815_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:55:26.82 +33:43:33.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 316817_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316817_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:09:40.57 +26:23:17.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 316818_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316818_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316821_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316821_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316828_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316828_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:24:48.32 +33:17:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.681 2055965561454641664 306.20104589390 +33.28812843856 13.5238 12.9717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316830_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316830_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:27:35.75 +32:14:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 316833_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316833_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:35:51.95 +30:42:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.403 2032730269447809792 293.96602726858 +30.71243586911 13.0829 12.5754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316834_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316834_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:51:31.19 +28:45:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.857 2028654139342845056 297.87969042159 +28.76090608937 13.3593 12.7837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316835_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316835_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316841_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316841_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:18:29.24 +31:18:59.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 316843_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316843_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:12.24 +26:04:38.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 316846_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316846_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:03:32.78 +31:43:36.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 316848_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316848_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:02:13.48 +32:29:13.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 316850_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316850_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316855_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316855_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316856_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316856_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:42.38 +28:36:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.663 2029103770834183936 301.17503738634 +28.61446189947 14.2524 13.1777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316857_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316857_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316860_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316860_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:13.61 +32:53:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.770 2046323840912350208 292.55535454689 +32.88423132741 12.6889 11.8276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316862_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316862_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:20.27 +33:04:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.064 2046336274829538176 292.58421121107 +33.06922350631 12.8739 12.1185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316863_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316863_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 316868_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316868_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:25:39.08 +30:52:07.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 316871_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316871_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:35:57.13 +32:19:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.946 2045306998835299200 293.98766764111 +32.32121859185 12.6759 11.8528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316872_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316872_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316877_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316877_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316884_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316884_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:47.54 +25:49:35.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 316886_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316886_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316887_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316887_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316889_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316889_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 316894_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316894_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316895_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316895_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316900_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316900_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:25:39.37 +33:51:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.121 2056019952921665920 306.41441743363 +33.85378104806 13.5910 12.9308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316904_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316904_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:50:45.92 +31:57:35.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 316906_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316906_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:36:33.26 +25:46:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.668 2021910830175020928 294.13763876284 +25.78268590370 13.3960 12.3639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316910_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316910_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:48:56.90 +33:44:41.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 316914_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316914_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316920_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316920_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:16.73 +29:39:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.204 2026599186448004992 292.56901807549 +29.66329424272 13.1823 12.6708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316923_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316923_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:54:20.14 +32:30:57.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 316924_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316924_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:33.58 +30:02:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.383 2032625708425052928 292.64023403376 +30.04099773460 13.2766 13.0619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316926_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316926_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:47.31 +31:09:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)
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Considering the candidate 316929_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316929_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316933_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316933_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316935_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316935_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316937_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316937_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316939_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316939_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316941_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316941_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316942_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316942_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316943_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316943_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316944_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316944_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:41:26.79 +33:26:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 316949_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316949_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316959_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316959_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:01.14 +32:07:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.472 2033284629467422464 295.75504520057 +32.11742973258 12.7219 12.0585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316966_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316966_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:29:25.75 +26:34:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.738 2024872708345691392 292.35813083828 +26.57807120199 13.1473 12.5535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316969_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316969_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:35:02.08 +31:55:43.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 316971_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316971_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316977_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316977_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316981_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316981_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 316985_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316985_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:00:14.18 +33:38:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 316990_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 316990_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 316996_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 316996_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:46:37.23 +30:14:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.947 2032116364008555392 296.65360088588 +30.23692084011 13.0400 12.5748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317006_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 317006_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:39:07.13 +33:43:56.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 317007_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317007_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317009_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317009_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317012_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317012_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317015_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317015_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317018_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 317018_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:33:12.64 +27:43:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.687 2025346632220163200 293.30252507060 +27.72494958256 12.8129 12.4657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317019_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317019_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317020_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317020_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317024_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317024_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317027_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317027_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317046_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 317046_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:38:46.08 +30:06:57.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)
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Considering the candidate 317713_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 317713_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 317911_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 317911_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 317972_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 317972_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:50.73 +28:27:40.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 318040_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318040_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 318046_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 318046_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 318169_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318169_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:21:33.49 +30:36:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318309_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 318309_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 318312_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318312_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:48:23.54 +27:18:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318354_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318354_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:49.93 +28:58:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318658_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318658_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:00:49.94 +32:59:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318677_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318677_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:06.85 +25:48:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318785_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 318785_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:50:48.25 +31:56:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147684_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 147684_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:39:22.96 +30:09:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188289_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 188289_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 294059_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 294059_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:13:25.78 +27:31:34.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 36668_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 36668_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 294664_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 294664_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 150655_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 150655_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 294826_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 294826_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:13:28.78 +29:38:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 109075_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 109075_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:29:15.86 +28:54:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186452_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 186452_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 154665_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 154665_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 102097_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 102097_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 228965_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 228965_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:42:53.14 +33:06:45.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 180224_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 180224_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 85590_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 85590_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:57.11 +28:32:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125090_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 125090_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:28:24.51 +29:22:30.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)
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Considering the candidate 198473_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 198473_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 110658_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 110658_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:52:10.13 +29:21:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35023_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 35023_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:32:08.29 +26:06:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124371_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 124371_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 45426_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 45426_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 180042_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 180042_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 83294_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 83294_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 22177_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 22177_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 31922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 31922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 234922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 234922_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 82978_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 82978_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 194937_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 194937_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 184305_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 184305_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 75595_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 75595_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 66542_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 66542_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 73692_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 73692_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:49:26.77 +28:05:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124732_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 124732_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 275068_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 275068_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:35:51.60 +33:56:19.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)
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Considering the candidate 152602_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 152602_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 25524_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 25524_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 132923_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 132923_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 221725_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 221725_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:54:57.22 +33:01:24.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
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Considering the candidate 53538_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 53538_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 278809_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 278809_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 191406_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 191406_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 43055_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 43055_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 295688_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 295688_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 242988_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 242988_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 295245_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 295245_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 236091_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 236091_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:57:07.55 +33:51:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294763_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 294763_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 90024_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 90024_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:33:52.23 +28:19:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77723_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 77723_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:32:02.07 +27:55:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294407_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
Preparing report for the candidate 294407_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
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Considering the candidate 293873_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 293873_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 60196_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 60196_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:51:30.94 +27:27:37.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 293756_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 293756_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:40.53 +26:51:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127342_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 127342_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:03:38.86 +29:53:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165195_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 165195_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:58:38.18 +30:59:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65096_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 65096_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:01:06.29 +27:45:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 200287_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 200287_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:04:36.14 +32:13:05.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 223982_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 223982_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:46:35.10 +32:53:15.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 89079_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 89079_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:14:14.51 +28:41:43.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160852_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 160852_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:09.77 +30:40:42.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65977_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 65977_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:15:45.92 +27:48:54.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212460_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 212460_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:42:44.76 +32:25:37.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 276916_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 276916_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:17.45 +33:43:42.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 236436_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 236436_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:46:26.04 +33:43:27.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255388_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 255388_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:34:56.46 +33:47:42.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 275957_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 275957_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:39:45.04 +33:58:44.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 48596_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 48596_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:31:21.86 +26:37:05.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25990_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 25990_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:43:43.09 +25:46:22.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 200523_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 200523_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 20:23:51.53 +32:11:23.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 88157_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 88157_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:30:44.25 +27:57:41.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 126219_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490
The candidate 126219_fd_Cyg-08-Q2b1x1_2026-03-27_05-34-17_20.00sec_-14.90C_LIGHT_0490 did not pass the final checks
**** FOUND 19:34:51.15 +29:27:48.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 18s
make_report_in_HTML.sh TOTAL: 143s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:03:39.70 +30:28:01.5
19:47:01.73 +28:37:58.4
19:48:19.02 +30:34:12.7
19:42:35.05 +28:56:19.4
19:40:30.82 +29:36:28.6
19:57:26.16 +29:50:23.6
20:00:05.84 +30:07:46.0
19:50:25.38 +30:34:07.2
19:45:33.78 +30:33:16.1
19:58:38.16 +30:48:00.8
19:51:30.22 +31:31:50.6
19:37:40.95 +31:17:34.0
20:02:44.55 +31:47:01.8
19:36:38.06 +31:30:02.9
19:43:14.55 +31:40:57.8
19:31:55.29 +31:33:45.0
19:32:14.14 +31:41:33.2
19:28:41.35 +31:44:00.8
19:59:06.37 +25:52:43.5
19:31:55.65 +33:29:48.7
19:34:48.00 +33:15:46.2
19:35:17.38 +25:42:29.2
19:27:15.07 +33:36:39.8
19:47:53.64 +32:03:00.1
19:54:40.86 +28:47:20.5
19:33:10.71 +30:07:50.3
19:38:04.23 +29:51:30.4
19:42:55.92 +33:40:49.7
19:54:41.81 +28:32:36.8
20:08:42.76 +33:33:27.5
20:13:26.50 +32:07:44.4
20:08:43.59 +33:33:25.2
20:13:59.19 +26:26:08.2
19:37:25.75 +33:58:20.5
19:48:09.87 +33:49:37.5
19:57:33.61 +32:57:34.9
19:31:37.14 +29:52:29.9
19:56:49.79 +33:00:47.9
19:31:03.49 +34:06:32.8
19:29:30.30 +27:46:13.5
19:52:08.28 +34:14:49.7
19:43:24.07 +33:13:14.0
19:48:28.45 +31:50:33.0
20:01:17.47 +33:37:09.4
20:24:47.02 +28:12:40.0
19:43:28.67 +33:25:16.8
19:54:08.89 +31:39:43.9
19:41:53.57 +29:12:34.6
19:57:16.49 +33:50:54.4
19:48:27.17 +30:53:12.3
19:45:21.72 +34:09:05.0
19:51:18.82 +31:56:40.9
19:43:07.55 +33:23:29.2
19:39:52.24 +31:14:35.2
19:32:27.33 +33:10:15.7
19:59:55.25 +29:20:05.7
19:50:45.43 +32:40:49.9
19:46:01.52 +33:42:32.4
19:45:58.26 +33:50:00.4
19:37:50.22 +32:17:10.0
19:39:52.38 +32:38:24.7
19:41:17.29 +31:25:36.6
19:34:11.64 +31:30:50.1
19:29:20.61 +31:43:41.6
19:42:46.51 +32:37:26.4
19:34:27.78 +26:01:01.0
19:40:08.55 +26:19:50.0
19:47:36.69 +26:45:43.4
20:10:05.70 +27:04:39.4
19:31:51.22 +26:56:58.7
19:29:48.75 +27:27:14.7
19:31:13.45 +27:49:32.6
19:39:53.07 +28:15:05.5
19:45:33.66 +28:21:29.8
########### Completed Cyg-08-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:03:39.70 +30:28:01.5
19:47:01.73 +28:37:58.4
19:48:19.02 +30:34:12.7
19:54:41.81 +28:32:36.8
20:08:42.76 +33:33:27.5
20:13:26.50 +32:07:44.4
20:08:43.59 +33:33:25.2
20:13:59.19 +26:26:08.2
19:37:25.75 +33:58:20.5
19:48:09.87 +33:49:37.5
19:57:33.61 +32:57:34.9
19:31:37.14 +29:52:29.9
19:56:49.79 +33:00:47.9
19:31:03.49 +34:06:32.8
19:29:30.30 +27:46:13.5
19:52:08.28 +34:14:49.7
19:43:24.07 +33:13:14.0
19:48:28.45 +31:50:33.0
20:01:17.47 +33:37:09.4
20:24:47.02 +28:12:40.0
19:43:28.67 +33:25:16.8
19:54:08.89 +31:39:43.9
19:41:53.57 +29:12:34.6
19:57:16.49 +33:50:54.4
19:48:27.17 +30:53:12.3
19:45:21.72 +34:09:05.0
19:51:18.82 +31:56:40.9
19:43:07.55 +33:23:29.2
19:39:52.24 +31:14:35.2
19:32:27.33 +33:10:15.7
19:59:55.25 +29:20:05.7
19:50:45.43 +32:40:49.9
19:46:01.52 +33:42:32.4
19:45:58.26 +33:50:00.4
19:37:50.22 +32:17:10.0
19:39:52.38 +32:38:24.7
19:41:17.29 +31:25:36.6
19:34:11.64 +31:30:50.1
19:29:20.61 +31:43:41.6
19:42:46.51 +32:37:26.4
19:43:14.55 +31:40:57.8
19:40:08.55 +26:19:50.0
19:54:40.86 +28:47:20.5
19:50:25.38 +30:34:07.2
19:36:38.06 +31:30:02.9
19:58:38.16 +30:48:00.8
19:42:35.05 +28:56:19.4
19:37:40.95 +31:17:34.0
19:28:41.35 +31:44:00.8
19:40:30.82 +29:36:28.6
20:10:05.70 +27:04:39.4
19:51:30.22 +31:31:50.6
19:45:33.66 +28:21:29.8
19:59:06.37 +25:52:43.5
19:34:27.78 +26:01:01.0
19:31:55.65 +33:29:48.7
19:39:53.07 +28:15:05.5
19:32:14.14 +31:41:33.2
20:02:44.55 +31:47:01.8
19:31:13.45 +27:49:32.6
19:29:48.75 +27:27:14.7
19:57:26.16 +29:50:23.6
19:45:33.78 +30:33:16.1
19:35:17.38 +25:42:29.2
20:00:05.84 +30:07:46.0
19:31:51.22 +26:56:58.7
19:27:15.07 +33:36:39.8
19:31:55.29 +31:33:45.0
19:47:36.69 +26:45:43.4
19:42:55.92 +33:40:49.7
19:34:48.00 +33:15:46.2
19:38:04.23 +29:51:30.4
19:33:10.71 +30:07:50.3
19:47:53.64 +32:03:00.1
###################################################################################
20:03:39.70 +30:28:01.5 -- not an asteroid (will add it to exclusion list)
19:47:01.73 +28:37:58.4 -- not an asteroid (will add it to exclusion list)
19:48:19.02 +30:34:12.7 -- not an asteroid (will add it to exclusion list)
19:54:41.81 +28:32:36.8 -- not an asteroid (will add it to exclusion list)
20:08:42.76 +33:33:27.5 -- not an asteroid (will add it to exclusion list)
20:13:26.50 +32:07:44.4 -- not an asteroid (will add it to exclusion list)
20:08:43.59 +33:33:25.2 -- not an asteroid (will add it to exclusion list)
20:13:59.19 +26:26:08.2 -- not an asteroid (will add it to exclusion list)
19:37:25.75 +33:58:20.5 -- not an asteroid (will add it to exclusion list)
19:48:09.87 +33:49:37.5 -- not an asteroid (will add it to exclusion list)
19:57:33.61 +32:57:34.9 -- not an asteroid (will add it to exclusion list)
19:31:37.14 +29:52:29.9 -- not an asteroid (will add it to exclusion list)
19:56:49.79 +33:00:47.9 -- not an asteroid (will add it to exclusion list)
19:31:03.49 +34:06:32.8 -- not an asteroid (will add it to exclusion list)
19:29:30.30 +27:46:13.5 -- not an asteroid (will add it to exclusion list)
19:52:08.28 +34:14:49.7 -- not an asteroid (will add it to exclusion list)
19:43:24.07 +33:13:14.0 -- not an asteroid (will add it to exclusion list)
19:48:28.45 +31:50:33.0 -- not an asteroid (will add it to exclusion list)
20:01:17.47 +33:37:09.4 -- not an asteroid (will add it to exclusion list)
20:24:47.02 +28:12:40.0 -- not an asteroid (will add it to exclusion list)
19:43:28.67 +33:25:16.8 -- not an asteroid (will add it to exclusion list)
19:54:08.89 +31:39:43.9 -- not an asteroid (will add it to exclusion list)
19:41:53.57 +29:12:34.6 -- not an asteroid (will add it to exclusion list)
19:57:16.49 +33:50:54.4 -- not an asteroid (will add it to exclusion list)
19:48:27.17 +30:53:12.3 -- not an asteroid (will add it to exclusion list)
19:45:21.72 +34:09:05.0 -- not an asteroid (will add it to exclusion list)
19:51:18.82 +31:56:40.9 -- not an asteroid (will add it to exclusion list)
19:43:07.55 +33:23:29.2 -- not an asteroid (will add it to exclusion list)
19:39:52.24 +31:14:35.2 -- not an asteroid (will add it to exclusion list)
19:32:27.33 +33:10:15.7 -- not an asteroid (will add it to exclusion list)
19:59:55.25 +29:20:05.7 -- not an asteroid (will add it to exclusion list)
19:50:45.43 +32:40:49.9 -- not an asteroid (will add it to exclusion list)
19:46:01.52 +33:42:32.4 -- not an asteroid (will add it to exclusion list)
19:45:58.26 +33:50:00.4 -- not an asteroid (will add it to exclusion list)
19:37:50.22 +32:17:10.0 -- not an asteroid (will add it to exclusion list)
19:39:52.38 +32:38:24.7 -- not an asteroid (will add it to exclusion list)
19:41:17.29 +31:25:36.6 -- not an asteroid (will add it to exclusion list)
19:34:11.64 +31:30:50.1 -- not an asteroid (will add it to exclusion list)
19:29:20.61 +31:43:41.6 -- not an asteroid (will add it to exclusion list)
19:42:46.51 +32:37:26.4 -- not an asteroid (will add it to exclusion list)
19:43:14.55 +31:40:57.8 -- not an asteroid (will add it to exclusion list)
19:40:08.55 +26:19:50.0 -- not an asteroid (will add it to exclusion list)
19:54:40.86 +28:47:20.5 -- not an asteroid (will add it to exclusion list)
19:50:25.38 +30:34:07.2 -- not an asteroid (will add it to exclusion list)
19:36:38.06 +31:30:02.9 -- not an asteroid (will add it to exclusion list)
19:58:38.16 +30:48:00.8 -- not an asteroid (will add it to exclusion list)
19:42:35.05 +28:56:19.4 -- not an asteroid (will add it to exclusion list)
19:37:40.95 +31:17:34.0 -- not an asteroid (will add it to exclusion list)
19:28:41.35 +31:44:00.8 -- not an asteroid (will add it to exclusion list)
19:40:30.82 +29:36:28.6 -- not an asteroid (will add it to exclusion list)
20:10:05.70 +27:04:39.4 -- not an asteroid (will add it to exclusion list)
19:51:30.22 +31:31:50.6 -- not an asteroid (will add it to exclusion list)
19:45:33.66 +28:21:29.8 -- not an asteroid (will add it to exclusion list)
19:59:06.37 +25:52:43.5 -- not an asteroid (will add it to exclusion list)
19:34:27.78 +26:01:01.0 -- not an asteroid (will add it to exclusion list)
19:31:55.65 +33:29:48.7 -- not an asteroid (will add it to exclusion list)
19:39:53.07 +28:15:05.5 -- not an asteroid (will add it to exclusion list)
19:32:14.14 +31:41:33.2 -- not an asteroid (will add it to exclusion list)
20:02:44.55 +31:47:01.8 -- not an asteroid (will add it to exclusion list)
19:31:13.45 +27:49:32.6 -- not an asteroid (will add it to exclusion list)
19:29:48.75 +27:27:14.7 -- not an asteroid (will add it to exclusion list)
19:57:26.16 +29:50:23.6 -- not an asteroid (will add it to exclusion list)
19:45:33.78 +30:33:16.1 -- not an asteroid (will add it to exclusion list)
19:35:17.38 +25:42:29.2 -- not an asteroid (will add it to exclusion list)
20:00:05.84 +30:07:46.0 -- not an asteroid (will add it to exclusion list)
19:31:51.22 +26:56:58.7 -- not an asteroid (will add it to exclusion list)
19:27:15.07 +33:36:39.8 -- not an asteroid (will add it to exclusion list)
19:31:55.29 +31:33:45.0 -- not an asteroid (will add it to exclusion list)
19:47:36.69 +26:45:43.4 -- not an asteroid (will add it to exclusion list)
19:42:55.92 +33:40:49.7 -- not an asteroid (will add it to exclusion list)
19:34:48.00 +33:15:46.2 -- not an asteroid (will add it to exclusion list)
19:38:04.23 +29:51:30.4 -- not an asteroid (will add it to exclusion list)
19:33:10.71 +30:07:50.3 -- not an asteroid (will add it to exclusion list)
19:47:53.64 +32:03:00.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:27:15.07 +33:36:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:41.35 +31:44:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:20.61 +31:43:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:30.30 +27:46:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:48.75 +27:27:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:03.49 +34:06:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:13.45 +27:49:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:37.14 +29:52:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:51.22 +26:56:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:55.29 +31:33:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:55.65 +33:29:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:14.14 +31:41:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:27.33 +33:10:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:10.71 +30:07:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:11.64 +31:30:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:27.78 +26:01:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:48.00 +33:15:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:17.38 +25:42:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:38.06 +31:30:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:25.75 +33:58:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:40.95 +31:17:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:50.22 +32:17:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:04.23 +29:51:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:52.24 +31:14:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:52.38 +32:38:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:53.07 +28:15:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:08.55 +26:19:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:30.82 +29:36:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:17.29 +31:25:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:53.57 +29:12:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:35.05 +28:56:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:46.51 +32:37:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:55.92 +33:40:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:07.55 +33:23:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:14.55 +31:40:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:24.07 +33:13:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:28.67 +33:25:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:21.72 +34:09:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:33.66 +28:21:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:33.78 +30:33:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:58.26 +33:50:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:01.52 +33:42:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:01.73 +28:37:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:36.69 +26:45:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:53.64 +32:03:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:09.87 +33:49:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:19.02 +30:34:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:27.17 +30:53:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:28.45 +31:50:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:25.38 +30:34:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:45.43 +32:40:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:18.82 +31:56:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:30.22 +31:31:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:08.28 +34:14:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:08.89 +31:39:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:40.86 +28:47:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:41.81 +28:32:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:49.79 +33:00:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:16.49 +33:50:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:26.16 +29:50:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:33.61 +32:57:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:38.16 +30:48:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:06.37 +25:52:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:55.25 +29:20:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:05.84 +30:07:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:17.47 +33:37:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:44.55 +31:47:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:39.70 +30:28:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:42.76 +33:33:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:43.59 +33:33:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:05.70 +27:04:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:26.50 +32:07:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:59.19 +26:26:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:47.02 +28:12:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:27:15.07 +33:36:39.8 -- not a known variable star
19:28:41.35 +31:44:00.8 -- not a known variable star
19:29:20.61 +31:43:41.6 -- a known variable star
19:29:30.30 +27:46:13.5 -- a known variable star
19:29:48.75 +27:27:14.7 -- not a known variable star
19:31:03.49 +34:06:32.8 -- not a known variable star
19:31:13.45 +27:49:32.6 -- not a known variable star
19:31:37.14 +29:52:29.9 -- not a known variable star
19:31:51.22 +26:56:58.7 -- not a known variable star
19:31:55.29 +31:33:45.0 -- not a known variable star
19:31:55.65 +33:29:48.7 -- not a known variable star
19:32:14.14 +31:41:33.2 -- not a known variable star
19:32:27.33 +33:10:15.7 -- not a known variable star
19:33:10.71 +30:07:50.3 -- not a known variable star
19:34:11.64 +31:30:50.1 -- not a known variable star
19:34:27.78 +26:01:01.0 -- a known variable star
19:34:48.00 +33:15:46.2 -- not a known variable star
19:35:17.38 +25:42:29.2 -- not a known variable star
19:36:38.06 +31:30:02.9 -- not a known variable star
19:37:25.75 +33:58:20.5 -- not a known variable star
19:37:40.95 +31:17:34.0 -- not a known variable star
19:37:50.22 +32:17:10.0 -- not a known variable star
19:38:04.23 +29:51:30.4 -- a known variable star
19:39:52.24 +31:14:35.2 -- not a known variable star
19:39:52.38 +32:38:24.7 -- not a known variable star
19:39:53.07 +28:15:05.5 -- not a known variable star
19:40:08.55 +26:19:50.0 -- not a known variable star
19:40:30.82 +29:36:28.6 -- not a known variable star
19:41:17.29 +31:25:36.6 -- a known variable star
19:41:53.57 +29:12:34.6 -- a known variable star
19:42:35.05 +28:56:19.4 -- a known variable star
19:42:46.51 +32:37:26.4 -- not a known variable star
19:42:55.92 +33:40:49.7 -- a known variable star
19:43:07.55 +33:23:29.2 -- not a known variable star
19:43:14.55 +31:40:57.8 -- not a known variable star
19:43:24.07 +33:13:14.0 -- a known variable star
19:43:28.67 +33:25:16.8 -- a known variable star
19:45:21.72 +34:09:05.0 -- not a known variable star
19:45:33.66 +28:21:29.8 -- a known variable star
19:45:33.78 +30:33:16.1 -- a known variable star
19:45:58.26 +33:50:00.4 -- a known variable star
19:46:01.52 +33:42:32.4 -- not a known variable star
19:47:01.73 +28:37:58.4 -- a known variable star
19:47:36.69 +26:45:43.4 -- a known variable star
19:47:53.64 +32:03:00.1 -- not a known variable star
19:48:09.87 +33:49:37.5 -- not a known variable star
19:48:19.02 +30:34:12.7 -- a known variable star
19:48:27.17 +30:53:12.3 -- a known variable star
19:48:28.45 +31:50:33.0 -- not a known variable star
19:50:25.38 +30:34:07.2 -- not a known variable star
19:50:45.43 +32:40:49.9 -- a known variable star
19:51:18.82 +31:56:40.9 -- not a known variable star
19:51:30.22 +31:31:50.6 -- a known variable star
19:52:08.28 +34:14:49.7 -- not a known variable star
19:54:08.89 +31:39:43.9 -- not a known variable star
19:54:40.86 +28:47:20.5 -- not a known variable star
19:54:41.81 +28:32:36.8 -- a known variable star
19:56:49.79 +33:00:47.9 -- not a known variable star
19:57:16.49 +33:50:54.4 -- not a known variable star
19:57:26.16 +29:50:23.6 -- a known variable star
19:57:33.61 +32:57:34.9 -- a known variable star
19:58:38.16 +30:48:00.8 -- a known variable star
19:59:06.37 +25:52:43.5 -- a known variable star
19:59:55.25 +29:20:05.7 -- a known variable star
20:00:05.84 +30:07:46.0 -- not a known variable star
20:01:17.47 +33:37:09.4 -- a known variable star
20:02:44.55 +31:47:01.8 -- not a known variable star
20:03:39.70 +30:28:01.5 -- a known variable star
20:08:42.76 +33:33:27.5 -- a known variable star
20:08:43.59 +33:33:25.2 -- a known variable star
20:10:05.70 +27:04:39.4 -- not a known variable star
20:13:26.50 +32:07:44.4 -- not a known variable star
20:13:59.19 +26:26:08.2 -- not a known variable star
20:24:47.02 +28:12:40.0 -- a known variable star
Found 44 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
74 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 74 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461126.94004984 -observatory 500
22:47:13.98 -08:14:34.7 Mercury (0.6mag)
01:36:02.44 +09:19:56.5 Venus (-3.9mag)
23:21:52.64 -05:15:23.2 Mars (1.2mag)
07:05:55.65 +22:56:29.8 Jupiter (-2.2mag)
00:20:18.06 -00:07:10.5 Saturn (0.9mag)
03:43:57.93 +19:35:18.9 Uranus (5.8mag)
00:08:11.16 -00:32:15.7 Neptune (7.8mag)
20:32:32.88 -22:53:03.6 Pluto (14.5mag)
08:01:29.98 +23:59:55.3 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Mar 27 07:19 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461126.94004984:
07:05:50.74 +22:56:41.2 Io (5.6mag)
07:05:52.97 +22:56:31.5 Europa (5.8mag)
07:05:43.59 +22:56:45.9 Ganymede (5.2mag)
07:06:12.34 +22:56:07.9 Callisto (6.5mag)
07:09:53.11 +22:54:22.9 Himalia (15.2mag)
07:05:57.63 +22:56:23.5 Thebe (16.1mag)
07:09:36.51 +23:20:16.4 Elara (17.2mag)
07:03:29.07 +23:46:46.1 Pasiphae (17.3mag)
07:14:37.52 +22:52:03.2 Carme (18.4mag)
00:20:29.77 -00:07:07.3 Titan (8.8mag)
00:20:17.90 -00:06:55.0 Rhea (10.1mag)
00:20:39.30 -00:04:58.7 Iapetus (11.5mag)
00:20:19.52 -00:06:46.5 Hyperion (14.8mag)
00:22:08.59 +00:03:33.3 Phoebe (16.8mag)
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461126.94004984:
13:40:43.38 +01:50:28.6 JWST
18:13:14.32 +31:30:30.1 Chandra
09:06:29.28 -48:54:39.4 XMM-Newton
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461126.94004984 -observatory 500
18:40:34.30 -27:45:15.0 14.0mag P/2010 H2 (Vales)
04:54:22.79 -70:40:15.7 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:15.72 +31:19:33.9 17.1mag C/2017 K2 (PANSTARRS)
17:30:28.64 +08:11:02.3 17.6mag C/2021 G2 (ATLAS)
23:03:59.89 +28:34:48.1 17.0mag C/2022 E2 (ATLAS)
04:07:16.53 +25:28:53.5 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.83 +31:40:28.8 16.1mag C/2022 QE78 (ATLAS)
08:29:48.74 -02:23:01.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:26.95 +16:50:51.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:31.21 -11:46:50.2 17.6mag P/2023 B1 (PANSTARRS)
09:19:25.39 -15:11:33.8 17.5mag C/2023 F3 (ATLAS)
21:30:57.07 +61:55:56.2 17.4mag C/2023 H5 (Lemmon)
19:31:10.26 -03:32:39.2 14.4mag C/2023 R1 (PANSTARRS)
21:40:53.73 +83:29:13.3 17.7mag C/2023 X2 (Lemmon)
06:14:00.00 +63:41:56.8 16.9mag C/2024 A1 (ATLAS)
04:25:45.15 +09:31:04.8 9.6mag C/2024 E1 (Wierzchos)
11:17:24.39 +03:59:19.4 18.0mag C/2024 G2 (ATLAS)
16:29:48.05 +03:11:20.6 17.4mag C/2024 G6 (ATLAS)
20:13:18.85 +10:16:09.9 14.8mag C/2024 J3 (ATLAS)
03:09:42.70 -25:32:27.2 16.4mag C/2024 T5 (ATLAS)
05:01:36.03 +50:37:00.9 17.6mag C/2025 J1 (Borisov)
14:54:34.93 +26:02:10.2 14.5mag C/2025 L1 (ATLAS)
02:56:48.45 -23:24:52.9 17.7mag C/2025 Q3 (ATLAS)
22:38:00.05 +19:26:41.5 11.6mag C/2025 R3 (PANSTARRS)
13:02:31.39 +01:44:35.0 17.6mag C/2025 Y1 (ATLAS)
01:50:51.81 -02:11:44.0 12.3mag C/2026 A1 (MAPS)
23:00:11.39 +32:52:17.1 13.9mag C/2026 B2 (Sun-Gao)
18:04:41.06 -10:37:47.8 12.9mag 10P/Tempel
15:22:39.28 +04:47:03.7 12.3mag 24P/Schaumasse
11:09:21.94 -02:13:54.7 15.6mag 29P/Schwassmann-Wachmann
17:49:44.94 -10:23:31.6 17.5mag 40P/Vaisala
10:42:05.81 -05:54:21.8 16.5mag 43P/Wolf-Harrington
01:18:40.91 +14:04:35.0 17.0mag 47P/Ashbrook-Jackson
06:37:43.80 +41:03:56.6 17.1mag 63P/Wild
23:03:08.62 -13:54:00.5 15.7mag 65P/Gunn
03:13:37.65 +13:57:18.2 15.9mag 76P/West-Kohoutek-Ikemura
00:23:07.84 +04:20:05.9 14.6mag 78P/Gehrels
22:00:39.42 -15:01:42.9 14.5mag 88P/Howell
01:17:15.69 +15:07:57.7 15.2mag 93P/Lovas
04:20:34.35 +31:06:41.7 16.4mag 123P/West-Hartley
08:10:32.36 +47:21:57.6 16.2mag 124P/Mrkos
02:03:41.83 +12:07:04.6 16.4mag 128P/Shoemaker-Holt
02:09:38.17 +11:56:19.4 17.4mag 131P/Mueller
23:49:05.29 +05:41:54.3 12.2mag 141P/Machholz
23:59:21.47 -02:17:40.8 12.3mag 141P-A/Machholz
22:55:57.96 -05:17:18.7 15.3mag 141P-D/Machholz
00:08:12.21 -11:08:21.7 15.4mag 162P/SidingSpring
10:35:18.43 +31:55:56.8 17.6mag 164P/Christensen
06:00:55.10 +24:41:18.8 17.6mag 198P/ODAS
15:24:26.21 -02:29:16.5 17.1mag 210P/Christensen
20:35:41.89 -16:07:24.7 17.2mag 218P/LINEAR
17:05:31.66 -16:05:19.2 16.2mag 235P/LINEAR
04:53:53.63 +32:48:21.1 16.4mag 240P/NEAT
07:31:09.78 -07:30:47.9 17.5mag 242P/Spahr
15:47:57.94 +05:35:09.7 17.6mag 391P/Kowalski
07:28:46.34 +21:12:20.4 17.6mag 450P/LONEOS
05:08:56.72 +46:12:22.6 17.3mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 27 07:20 tocp_transients_list.txt