This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e
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
KID 5019263,2461126.8949,13.18,0.05,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
KID 5019263 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:25.80 +40:10:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 13.01 19:37:59.60 +41:41:08.3
75.01745 9.73907 galactic Cyg Second-epoch detections are separated by 4.1" and 6.9 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 J294.4925+41.6889 | 19:37:59.60 +41:41:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.4925+41.6889,2461126.8949,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.4925+41.6889 20260327.3949 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:59.60 +41:41:08.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.8949,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3949 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:36.83 +35:29:58.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.95 19:27:51.60 +39:46:14.6
72.39570 10.57059 galactic Lyr Second-epoch detections are separated by 0.8" and 7.0 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 J291.9580+39.7672 | 19:27:51.60 +39:46:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M5III 2016AJ....151...13G LAMOST J192750.35+394615.0
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J291.9580+39.7672,2461126.8949,12.95,0.05,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 J291.9580+39.7672 20260327.3949 12.95CV 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:27:51.60 +39:46:14.6 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.88 19:40:23.98 +38:09:00.0
72.08721 7.65952 galactic Cyg Second-epoch detections are separated by 7.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.0924+38.1506 | 19:40:23.98 +38:09:00.0 (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 J295.0924+38.1506,2461126.8949,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.0924+38.1506 20260327.3949 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:23.98 +38:09:00.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.93 19:49:17.81 +33:50:35.7
69.20799 3.97432 galactic Cyg Second-epoch detections are separated by 3.1" and 8.0 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 J297.3186+33.8453 | 19:49:17.81 +33:50:35.7 (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 J297.3186+33.8453,2461126.8949,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.3186+33.8453 20260327.3949 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:17.81 +33:50:35.7 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.94 20:07:24.46 +40:48:60.0
77.05544 4.52236 galactic Cyg Second-epoch detections are separated by 1.9" and 7.2 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 J301.8556+40.8097 | 20:07:24.46 +40:48:60.0 (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 J301.8556+40.8097,2461126.8949,12.94,0.05,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 J301.8556+40.8097 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:24.46 +40:48:60.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 6790426,2461126.8949,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KIC 6790426 20260327.3949 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:38.52 +42:15:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.8949,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3949 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:13.43 +39:08:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.86 19:32:59.84 +42:12:10.6
75.04973 10.80190 galactic Cyg Second-epoch detections are separated by 5.4" and 6.4 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 J293.2513+42.2095 | 19:32:59.84 +42:12:10.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F3Ia 2016AJ....151...13G LAMOST J193300.33+421234.4
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J293.2513+42.2095,2461126.8949,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2513+42.2095 20260327.3949 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:59.84 +42:12:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.80 19:59:38.69 +39:02:21.0
74.75248 4.84717 galactic Cyg Second-epoch detections are separated by 4.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9059+39.0412 | 19:59:38.69 +39:02:21.0 (user input) | dubious (ATLAS) | (ATLAS) | (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
ATO J299.9059+39.0412,2461126.8949,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9059+39.0412 20260327.3949 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:38.69 +39:02:21.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.8949,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3949 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:04.03 +40:34:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.79 20:01:11.41 +40:12:29.3
75.90954 5.20288 galactic Cyg Second-epoch detections are separated by 0.3" and 7.5 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 J300.2907+40.2192 | 20:01:11.41 +40:12:29.3 (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 J300.2907+40.2192,2461126.8949,12.79,0.05,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 J300.2907+40.2192 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:11.41 +40:12:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.79 19:24:51.67 +34:41:28.0
67.52350 8.81139 galactic Lyr Second-epoch detections are separated by 2.0" and 7.2 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 J291.2044+34.6994 | 19:24:51.67 +34:41:28.0 (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 J291.2044+34.6994,2461126.8949,12.79,0.05,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 J291.2044+34.6994 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:24:51.67 +34:41:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.71 19:54:27.67 +35:29:17.1
71.16882 3.89573 galactic Cyg Second-epoch detections are separated by 1.9" and 7.8 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 J298.6147+35.4948 | 19:54:27.67 +35:29:17.1 (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 J298.6147+35.4948,2461126.8949,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.6147+35.4948 20260327.3949 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:27.67 +35:29:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2050648971750908928,2461126.8949,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2050648971750908928 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:54.96 +35:55:50.1 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 5455870,2461126.8949,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KIC 5455870 20260327.3949 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:58.99 +40:37:30.3 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.46 19:58:47.01 +35:30:44.9
71.64560 3.15545 galactic Cyg Second-epoch detections are separated by 2.1" and 7.8 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 J299.6925+35.5120 | 19:58:47.01 +35:30:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6925+35.5120,2461126.8949,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6925+35.5120 20260327.3949 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:47.01 +35:30:44.9 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2047035328001110912,2461126.8949,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2047035328001110912 20260327.3949 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:00.51 +33:49:36.6 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.70 19:57:24.21 +41:09:40.0
76.35553 6.31037 galactic Cyg Second-epoch detections are separated by 1.9" and 7.4 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 J299.3530+41.1627 | 19:57:24.21 +41:09:40.0 (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 J299.3530+41.1627,2461126.8949,12.70,0.05,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
ATO J299.3530+41.1627 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:24.21 +41:09:40.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.8949,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3949 12.95CV 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:51.65 +41:55:01.5 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.95 19:39:51.76 +34:12:15.6
68.55348 5.85211 galactic Cyg Second-epoch detections are separated by 2.5" and 7.4 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 J294.9626+34.2048 | 19:39:51.76 +34:12:15.6 (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 J294.9626+34.2048,2461126.8949,12.95,0.05,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 J294.9626+34.2048 20260327.3949 12.95CV 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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:51.76 +34:12:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.85 20:01:33.10 +36:29:01.4
72.76792 3.18784 galactic Cyg Second-epoch detections are separated by 3.8" and 7.9 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 J300.3800+36.4779 | 20:01:33.10 +36:29:01.4 (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 J300.3800+36.4779,2461126.8949,12.85,0.05,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
ATO J300.3800+36.4779 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:01:33.10 +36:29:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 5027715,2461126.8949,12.91,0.05,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
KIC 5027715 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:55.09 +40:06:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2060181776265047040,2461126.8949,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2060181776265047040 20260327.3949 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:02.51 +37:20:38.6 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195746.70+365258.8,2461126.8949,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195746.70+365258.8 20260327.3949 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:45.83 +36:52:44.0 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 11.26 19:59:19.48 +38:29:24.0
74.24933 4.61471 galactic Cyg Second-epoch detections are separated by 0.7" and 7.5 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 J299.8409+38.4914 | 19:59:19.80 +38:29:16.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8: 1949ApJ...110..478N LF 3b +38 118
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.8409+38.4914,2461126.8949,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8409+38.4914 20260327.3949 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:19.48 +38:29:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.54 19:04:26.08 +40:57:26.3
71.57849 15.11760 galactic Lyr Second-epoch detections are separated by 3.7" and 7.7 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 J286.1151+40.9598 | 19:04:25.51 +40:57:23.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.1151+40.9598,2461126.8949,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.1151+40.9598 20260327.3949 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:04:26.08 +40:57:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 11.92 19:06:43.66 +38:19:04.0
69.26092 13.66062 galactic Lyr Second-epoch detections are separated by 1.4" and 7.6 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 2099229449911277056 | 19:06:44.23 +38:19:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2099229449911277056,2461126.8949,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2099229449911277056 20260327.3949 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:43.66 +38:19:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.26 19:49:35.94 +34:50:59.1
70.11140 4.42728 galactic Cyg Second-epoch detections are separated by 2.6" and 7.3 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 J297.3956+34.8435 | 19:49:35.94 +34:50:59.1 (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 J297.3956+34.8435,2461126.8949,12.26,0.05,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 J297.3956+34.8435 20260327.3949 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:35.94 +34:50:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2072797018584831360,2461126.8949,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2072797018584831360 20260327.3949 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:15.67 +37:37:13.2 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.45 20:07:07.31 +41:15:00.4
77.39374 4.80000 galactic Cyg Second-epoch detections are separated by 1.6" and 7.4 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 J301.7838+41.2512 | 20:07:08.13 +41:15:04.5 (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 J301.7838+41.2512,2461126.8949,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.7838+41.2512 20260327.3949 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:07.31 +41:15:00.4 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.68 19:13:13.44 +34:34:38.1
66.34472 10.90758 galactic Lyr Second-epoch detections are separated by 6.7" and 6.5 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 J288.2956+34.5686 | 19:13:13.44 +34:34:38.1 (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 J288.2956+34.5686,2461126.8949,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.2956+34.5686 20260327.3949 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:13:13.44 +34:34:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.33 19:41:18.56 +40:09:36.8
73.95518 8.46665 galactic Cyg Second-epoch detections are separated by 6.2" and 8.1 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 J295.3322+40.1618 | 19:41:18.56 +40:09:36.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G9III 2016A&A...594A..39F KIC 5024476
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J295.3322+40.1618,2461126.8949,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.3322+40.1618 20260327.3949 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:18.56 +40:09:36.8 ;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-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 3237523,2461126.8949,12.39,0.05,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
KIC 3237523 20260327.3949 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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:15.40 +38:17:60.0 ;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-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461126.8949,12.47,0.05,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
target 20260327.3949 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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:05.46 +34:08:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04426,2461126.8949,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04426 20260327.3949 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:53:23.66 +37:26:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.62 19:57:41.02 +36:01:16.8
71.96461 3.61075 galactic Cyg Second-epoch detections are separated by 4.4" and 8.1 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 J299.4207+36.0235 | 19:57:41.02 +36:01:16.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.446+/-0.046 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4207+36.0235,2461126.8949,12.62,0.05,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
ATO J299.4207+36.0235 20260327.3949 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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:41.02 +36:01:16.8 ;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-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2072500631485537664,2461126.8949,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2072500631485537664 20260327.3949 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:15.22 +37:58:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3949 2461126.8949 12.82 19:46:41.25 +35:46:36.1
70.61916 5.40506 galactic Cyg Second-epoch detections are separated by 2.6" and 7.2 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 J296.6728+35.7783 | 19:46:41.25 +35:46:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.848+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.6728+35.7783,2461126.8949,12.82,0.05,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 J296.6728+35.7783 20260327.3949 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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:41.25 +35:46:36.1 ;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-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20_00sec_-15_00C_LIGHT_0417_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20_00sec_-14_90C_LIGHT_0416_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: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461126.89514284 27.03.2026 09:28:50.341 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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: 7 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): 27878
Objects passed selection criteria: 27792
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 22318.5
Average stars matched: 21627.2 (96.9028 %)
Memory usage VmPeak: 133516 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 05:28:55 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: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461126.89514284 27.03.2026 09:28:50.341 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 239
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 81 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): 235967
Objects passed selection criteria: 235282
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 166455
Average stars matched: 159336 (95.7232 %)
Memory usage VmPeak: 1997380 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 05:36:40 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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: 2461126.89458705
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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits'
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:37:49.266 +38:02:47.21
Angular distance between the image centers 0.13 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:37:46.236 +38:02:25.10
Angular distance between the image centers 0.13 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 19:37:49.266 +38:02:47.21
Second-epoch second image center 19:37:46.236 +38:02:25.10
Angular distance between the image centers 0.01169 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.GgYuJ0lA5h
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.eqk47B5zpN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.6GUAve99kv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits &> /tmp/tmp.mmezLFUyfK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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 2233 out of 36462 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.855034
a=0.000000 b=1.000000 c=22.855034
From vast_summary.log: estimated ref. image limiting mag.: -7.84
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 46 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
2.2 pix Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
4.2 pix fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
5.5 pix fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Limiting magnitude estimates:
15.0 mag. Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.0 mag. Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
14.0 mag. fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
13.8 mag. fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GgYuJ0lA5h (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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4454, passed=36462
Got 36462 stars (including 31968 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 36462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 851 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: 2.11"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.31"
Estimated accuracy of the plate solution: 1.31"
Excluding outliers - 896 stars left (next iteration limit 907)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.eqk47B5zpN (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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4450, passed=36391
Got 36391 stars (including 31905 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 36391 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 920 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: 2.11"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.16"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.13"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 912 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.6GUAve99kv (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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1185, passed=19406
Got 19406 stars (including 18216 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 19406 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 940 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: 0.92"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.88"
Estimated accuracy of the plate solution: 1.09"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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.mmezLFUyfK (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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=897, passed=15776
Got 15776 stars (including 14878 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 15776 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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.01"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.02"
Estimated accuracy of the plate solution: 1.25"
Excluding outliers - 925 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-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
Saving fully-calibrated image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits'
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52559_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 52559_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:20:08.95 +41:40:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52570_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 52570_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:09.75 +39:47:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14813_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 14813_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:07:18.29 +36:06:04.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24873_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 24873_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:13:45.90 +39:08:49.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21266_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 21266_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:16:22.63 +38:08:05.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08308_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 08308_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:56:18.41 +35:05:06.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06870_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 06870_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:31:46.65 +34:27:16.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20990_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 20990_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:55:51.98 +38:29:16.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14171_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 14171_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:26:09.42 +36:19:07.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21501_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 21501_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:34.16 +38:43:28.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08429_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 08429_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:45:51.53 +35:00:50.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17112_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 17112_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:17.04 +37:21:21.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08074_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 08074_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:31:31.42 +34:42:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12886_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 12886_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:00:13.39 +36:08:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28134_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 28134_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:53.81 +40:15:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22568_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 22568_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:33:36.55 +38:45:45.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21182_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 21182_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:36:56.76 +38:23:03.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09580_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 09580_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:38:01.56 +35:15:32.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21888_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 21888_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:10.89 +38:40:20.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19004_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 19004_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:22:40.97 +37:34:54.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19953_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 19953_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:27:36.54 +37:56:29.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13692_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 13692_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:30:46.99 +36:13:44.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27014_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 27014_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:41:57.61 +40:15:19.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14828_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 14828_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:24:06.13 +36:27:10.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15983_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 15983_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:35:48.53 +36:56:43.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24605_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 24605_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:17:20.12 +39:07:15.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21887_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 21887_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:49:27.57 +38:42:41.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08572_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 08572_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:37:40.89 +35:01:22.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18304_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 18304_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:38.99 +37:19:46.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20894_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 20894_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:47:27.83 +38:24:32.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12574_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 12574_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:45:40.09 +36:05:27.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18816_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 18816_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:01.22 +37:26:45.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13601_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 13601_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:52:16.52 +36:25:58.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10355_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 10355_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:20:33.05 +35:11:10.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28278_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 28278_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:49.05 +40:43:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05356_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 05356_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:51.65 +34:09:48.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04814_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 04814_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:39:44.96 +33:58:46.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18607_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 18607_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:47.00 +37:49:37.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15673_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 15673_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:54:48.35 +36:59:46.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13067_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 13067_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:56:44.24 +36:15:04.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27880_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 27880_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:37.51 +40:36:01.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28770_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 28770_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:11:23.18 +40:25:45.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33426_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 33426_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:45.30 +41:46:24.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05946_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 05946_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:38.26 +34:24:53.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27197_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 27197_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:57:14.10 +40:22:07.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15876_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 15876_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:59:55.41 +37:02:37.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Cyg-05-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 ####
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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits exists and is non-empty
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:37:49.266 +38:02:47.21
Angular distance between the image centers 0.13 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:37:46.236 +38:02:25.10
Angular distance between the image centers 0.13 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 19:37:49.266 +38:02:47.21
Second-epoch second image center 19:37:46.236 +38:02:25.10
Angular distance between the image centers 0.01169 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.QyKzJe1RQK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.MsZl6AYCN7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.kwzuT9AlWJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits &> /tmp/tmp.zMPak5g3RV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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 2470 out of 289933 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.659513
a=0.000000 b=1.000000 c=22.659513
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 150 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
1.9 pix Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
4.3 pix fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
5.8 pix fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Limiting magnitude estimates:
15.2 mag. Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.2 mag. Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
14.1 mag. fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
13.9 mag. fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 12.9 (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.QyKzJe1RQK (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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=54567, passed=289884
Got 289884 stars (including 234962 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 289884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 835 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: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.33"
Estimated accuracy of the plate solution: 1.37"
Excluding outliers - 887 stars left (next iteration limit 889)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.MsZl6AYCN7 (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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=55059, passed=293495
Got 293495 stars (including 238063 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 293495 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.07"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.15"
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 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.14"
Estimated accuracy of the plate solution: 1.22"
Excluding outliers - 897 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.kwzuT9AlWJ (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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=15224, passed=98648
Got 98648 stars (including 83377 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 98648 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 935 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: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 924 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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.zMPak5g3RV (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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=11788, passed=73074
Got 73074 stars (including 61258 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 73074 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: 1.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.02"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.02"
Estimated accuracy of the plate solution: 1.30"
Excluding outliers - 920 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Saving fully-calibrated image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-02_20.00sec_-14.90C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.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-05-Q2b1x1_052338_TTUQ2b1x1_22131_n8anw95e/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417.fits
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out218572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66074.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 56s
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: 22s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325974_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 325974_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:06:05.32 +41:49:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.820 2103946290375685888 286.52174189050 +41.82222743474 13.0805 12.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325982_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 325982_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325996_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 325996_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:14:54.97 +41:00:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.619 2102104024284493696 288.72954329333 +41.00314624113 12.9417 12.4902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326009_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326009_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:36:52.50 +41:25:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326013_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326013_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326017_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326017_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326019_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326019_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:37:12.22 +38:48:08.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326024_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326024_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326025_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326025_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326027_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326027_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326028_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326028_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:05.81 +35:59:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.199 2047844293707369088 296.02437778226 +35.98289560505 12.9118 12.0692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326029_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326029_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326034_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326034_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326038_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326038_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326049_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326049_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:57:01.90 +40:11:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326050_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326050_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326053_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326053_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326055_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326055_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326056_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326056_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:56:46.53 +37:12:06.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326063_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326063_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326064_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326064_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326073_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326073_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326081_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326081_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326083_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326083_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326085_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326085_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326096_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326096_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326100_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 326100_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326104_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 326104_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327063_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 327063_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327097_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 327097_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 327132_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 327132_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:39:35.64 +33:59:24.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209361_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 209361_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:13:45.86 +39:08:49.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181120_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 181120_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:16:22.63 +38:08:05.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56499_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 56499_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:31:46.64 +34:27:16.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175993_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 175993_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:55:51.98 +38:29:16.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186268_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 186268_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:34.16 +38:43:26.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144424_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 144424_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:17.03 +37:21:21.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30467_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 30467_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303405_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 303405_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:48:11.57 +34:58:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246141_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 246141_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99753_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 99753_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:00:13.42 +36:08:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210606_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 210606_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:09.51 +39:47:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270282_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 270282_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188769_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 188769_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:51:49.10 +39:00:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102690_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 102690_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:59:53.53 +36:16:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128872_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 128872_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:55:19.62 +37:03:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276789_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 276789_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:20:08.94 +41:40:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302371_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 302371_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116539_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 116539_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:02:26.24 +36:42:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.714 2059938092657765632 300.61035103231 +36.70281303943 13.2832 12.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109239_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 109239_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279036_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 279036_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:02:28.85 +41:18:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218572_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 218572_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127418_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 127418_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:07:49.26 +36:23:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50682_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 50682_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:09:26.93 +33:56:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232006_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 232006_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:53.78 +40:15:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233771_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 233771_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:47:34.88 +40:44:09.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137046_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 137046_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122382_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 122382_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161477_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 161477_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:02:56.56 +38:07:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81331_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 81331_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222848_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 222848_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:45:26.05 +40:15:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76078_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 76078_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61065_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 61065_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:31:31.42 +34:42:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172664_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 172664_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215082_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 215082_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284277_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 284277_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187381_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 187381_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59122_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 59122_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40652_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 40652_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51759_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 51759_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:40:55.49 +34:31:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248978_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 248978_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:04:22.26 +41:02:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147142_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 147142_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243364_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 243364_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40574_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 40574_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:09.20 +34:10:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66074_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 66074_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60849_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 60849_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:15:56.85 +34:27:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304347_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 304347_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303946_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 303946_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:55:17.12 +33:59:48.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303841_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 303841_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303715_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 303715_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303565_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 303565_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303562_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 303562_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303341_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 303341_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:49:47.65 +34:58:34.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157051_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 157051_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303022_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
Preparing report for the candidate 303022_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302983_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 302983_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:02:02.96 +41:04:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.609 2103850078809355264 285.51103676034 +41.07730465164 12.3172 11.8106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204204_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 204204_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:59.69 +39:33:55.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171959_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 171959_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:47.13 +38:19:20.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181644_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 181644_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:37:17.61 +38:35:40.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113768_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 113768_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:25:58.03 +36:11:12.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174982_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 174982_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:36:56.76 +38:23:03.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218659_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 218659_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:04.28 +39:59:54.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187223_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 187223_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:33:36.55 +38:45:45.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218704_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 218704_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:41:39.66 +40:01:25.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220754_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 220754_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:28:38.49 +39:56:26.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214428_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 214428_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:23:47.90 +39:35:26.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302575_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 302575_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:13:17.82 +37:03:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182674_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 182674_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:10.97 +38:40:20.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235937_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 235937_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:42:56.25 +40:43:19.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131788_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 131788_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:35:48.53 +36:56:43.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146804_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 146804_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:25:18.21 +37:14:42.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76844_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 76844_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:36:07.46 +35:12:48.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113368_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 113368_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:29:30.06 +36:17:18.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167683_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 167683_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:27:36.48 +37:56:30.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173848_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 173848_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:47:27.92 +38:24:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79348_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 79348_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:38:01.56 +35:15:32.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226310_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 226310_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:41:57.53 +40:15:21.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75892_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 75892_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:48:44.03 +35:18:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110717_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 110717_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:30:46.92 +36:13:44.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224429_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 224429_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:20:27.14 +39:55:34.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182268_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 182268_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:49:27.61 +38:42:37.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101247_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 101247_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:45:40.09 +36:05:28.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173898_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 173898_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:57:29.06 +38:27:31.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159231_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 159231_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:46.99 +37:49:38.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158446_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 158446_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:22:40.96 +37:34:54.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123604_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 123604_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:24:06.10 +36:27:09.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72044_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 72044_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:37:40.85 +35:01:23.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235285_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 235285_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:18:58.06 +40:21:38.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276093_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 276093_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:34:18.15 +41:55:38.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111692_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 111692_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:52:16.50 +36:25:58.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203867_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 203867_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:17:09.23 +39:01:44.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236846_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 236846_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:49.02 +40:43:01.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68745_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 68745_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:45:51.53 +35:00:50.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117634_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 117634_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:26:09.49 +36:19:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221701_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 221701_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:55:40.54 +40:10:24.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129101_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 129101_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:54:48.34 +36:59:47.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162764_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 162764_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:58:34.41 +38:06:22.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151718_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 151718_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:38.98 +37:19:46.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232930_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 232930_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:50:37.49 +40:36:01.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155919_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 155919_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:19:01.23 +37:26:45.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205351_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 205351_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:17:20.08 +39:07:16.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38771_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 38771_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:39:44.97 +33:58:46.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44456_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 44456_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:51.59 +34:09:48.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52283_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 52283_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:44:38.26 +34:24:54.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302469_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 302469_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:32:42.65 +34:20:49.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36538_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 36538_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:34:56.17 +33:47:47.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302467_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 302467_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:07:17.76 +40:23:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.041 2100793509502529664 286.82226688885 +40.39000504013 13.7970 12.8454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171962_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 171962_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:09:45.99 +37:47:40.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106363_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 106363_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:56:44.24 +36:15:04.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 279687_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 279687_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:43:45.29 +41:46:25.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82510_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 82510_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:20:33.19 +35:11:11.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130322_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 130322_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:59:55.39 +37:02:38.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131938_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 131938_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:01:15.35 +37:05:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226806_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 226806_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:57:14.09 +40:22:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107752_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 107752_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:09:56.40 +35:39:41.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174981_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 174981_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 20:05:10.18 +38:28:45.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275390_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 275390_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:06:16.90 +41:24:50.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74654_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 74654_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:09:04.20 +34:36:07.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250232_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 250232_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:11:23.17 +40:25:45.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122586_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417
The candidate 122586_fd_Cyg-05-Q2b1x1_2026-03-27_04-28-50_20.00sec_-15.00C_LIGHT_0417 did not pass the final checks
**** FOUND 19:07:18.29 +36:06:04.3 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 89s
Prepared the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:01:33.10 +36:29:01.4
19:57:45.83 +36:52:44.0
20:02:02.51 +37:20:38.6
19:47:15.67 +37:37:13.2
19:55:15.22 +37:58:47.3
19:59:19.48 +38:29:24.0
19:06:43.66 +38:19:04.0
19:43:55.09 +40:06:41.7
20:07:07.31 +41:15:00.4
19:57:24.21 +41:09:40.0
19:57:51.65 +41:55:01.5
19:04:26.08 +40:57:26.3
19:39:51.76 +34:12:15.6
19:46:41.25 +35:46:36.1
19:57:41.02 +36:01:16.8
19:53:23.66 +37:26:33.4
19:32:05.46 +34:08:21.6
19:28:15.40 +38:17:60.0
19:41:18.56 +40:09:36.8
19:44:00.51 +33:49:36.6
19:36:25.80 +40:10:57.4
19:37:59.60 +41:41:08.3
19:52:36.83 +35:29:58.0
19:27:51.60 +39:46:14.6
19:40:23.98 +38:09:00.0
19:49:17.81 +33:50:35.7
20:07:24.46 +40:48:60.0
19:41:38.52 +42:15:45.4
20:01:13.43 +39:08:56.1
19:32:59.84 +42:12:10.6
19:59:38.69 +39:02:21.0
20:01:04.03 +40:34:52.4
20:01:11.41 +40:12:29.3
19:24:51.67 +34:41:28.0
19:54:27.67 +35:29:17.1
19:08:54.96 +35:55:50.1
19:35:58.99 +40:37:30.3
19:58:47.01 +35:30:44.9
19:49:35.94 +34:50:59.1
19:13:13.44 +34:34:38.1
########### Completed Cyg-05-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 ####
19:36:25.80 +40:10:57.4
19:37:59.60 +41:41:08.3
19:52:36.83 +35:29:58.0
19:27:51.60 +39:46:14.6
19:40:23.98 +38:09:00.0
19:49:17.81 +33:50:35.7
20:07:24.46 +40:48:60.0
19:41:38.52 +42:15:45.4
20:01:13.43 +39:08:56.1
19:32:59.84 +42:12:10.6
19:59:38.69 +39:02:21.0
20:01:04.03 +40:34:52.4
20:01:11.41 +40:12:29.3
19:24:51.67 +34:41:28.0
19:54:27.67 +35:29:17.1
19:08:54.96 +35:55:50.1
19:35:58.99 +40:37:30.3
19:58:47.01 +35:30:44.9
19:44:00.51 +33:49:36.6
19:57:24.21 +41:09:40.0
19:57:51.65 +41:55:01.5
19:39:51.76 +34:12:15.6
20:01:33.10 +36:29:01.4
19:43:55.09 +40:06:41.7
20:02:02.51 +37:20:38.6
19:57:45.83 +36:52:44.0
19:59:19.48 +38:29:24.0
19:04:26.08 +40:57:26.3
19:06:43.66 +38:19:04.0
19:49:35.94 +34:50:59.1
19:47:15.67 +37:37:13.2
20:07:07.31 +41:15:00.4
19:13:13.44 +34:34:38.1
19:41:18.56 +40:09:36.8
19:28:15.40 +38:17:60.0
19:32:05.46 +34:08:21.6
19:53:23.66 +37:26:33.4
19:57:41.02 +36:01:16.8
19:55:15.22 +37:58:47.3
19:46:41.25 +35:46:36.1
###################################################################################
19:36:25.80 +40:10:57.4 -- not an asteroid (will add it to exclusion list)
19:37:59.60 +41:41:08.3 -- not an asteroid (will add it to exclusion list)
19:52:36.83 +35:29:58.0 -- not an asteroid (will add it to exclusion list)
19:27:51.60 +39:46:14.6 -- not an asteroid (will add it to exclusion list)
19:40:23.98 +38:09:00.0 -- not an asteroid (will add it to exclusion list)
19:49:17.81 +33:50:35.7 -- not an asteroid (will add it to exclusion list)
20:07:24.46 +40:48:60.0 -- not an asteroid (will add it to exclusion list)
19:41:38.52 +42:15:45.4 -- not an asteroid (will add it to exclusion list)
20:01:13.43 +39:08:56.1 -- not an asteroid (will add it to exclusion list)
19:32:59.84 +42:12:10.6 -- not an asteroid (will add it to exclusion list)
19:59:38.69 +39:02:21.0 -- not an asteroid (will add it to exclusion list)
20:01:04.03 +40:34:52.4 -- not an asteroid (will add it to exclusion list)
20:01:11.41 +40:12:29.3 -- not an asteroid (will add it to exclusion list)
19:24:51.67 +34:41:28.0 -- not an asteroid (will add it to exclusion list)
19:54:27.67 +35:29:17.1 -- not an asteroid (will add it to exclusion list)
19:08:54.96 +35:55:50.1 -- not an asteroid (will add it to exclusion list)
19:35:58.99 +40:37:30.3 -- not an asteroid (will add it to exclusion list)
19:58:47.01 +35:30:44.9 -- not an asteroid (will add it to exclusion list)
19:44:00.51 +33:49:36.6 -- not an asteroid (will add it to exclusion list)
19:57:24.21 +41:09:40.0 -- not an asteroid (will add it to exclusion list)
19:57:51.65 +41:55:01.5 -- not an asteroid (will add it to exclusion list)
19:39:51.76 +34:12:15.6 -- not an asteroid (will add it to exclusion list)
20:01:33.10 +36:29:01.4 -- not an asteroid (will add it to exclusion list)
19:43:55.09 +40:06:41.7 -- not an asteroid (will add it to exclusion list)
20:02:02.51 +37:20:38.6 -- not an asteroid (will add it to exclusion list)
19:57:45.83 +36:52:44.0 -- not an asteroid (will add it to exclusion list)
19:59:19.48 +38:29:24.0 -- not an asteroid (will add it to exclusion list)
19:04:26.08 +40:57:26.3 -- not an asteroid (will add it to exclusion list)
19:06:43.66 +38:19:04.0 -- not an asteroid (will add it to exclusion list)
19:49:35.94 +34:50:59.1 -- not an asteroid (will add it to exclusion list)
19:47:15.67 +37:37:13.2 -- not an asteroid (will add it to exclusion list)
20:07:07.31 +41:15:00.4 -- not an asteroid (will add it to exclusion list)
19:13:13.44 +34:34:38.1 -- not an asteroid (will add it to exclusion list)
19:41:18.56 +40:09:36.8 -- not an asteroid (will add it to exclusion list)
19:28:15.40 +38:17:60.0 -- not an asteroid (will add it to exclusion list)
19:32:05.46 +34:08:21.6 -- not an asteroid (will add it to exclusion list)
19:53:23.66 +37:26:33.4 -- not an asteroid (will add it to exclusion list)
19:57:41.02 +36:01:16.8 -- not an asteroid (will add it to exclusion list)
19:55:15.22 +37:58:47.3 -- not an asteroid (will add it to exclusion list)
19:46:41.25 +35:46:36.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:04:26.08 +40:57:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:43.66 +38:19:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:54.96 +35:55:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:13.44 +34:34:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:51.67 +34:41:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:51.60 +39:46:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:15.40 +38:17:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:05.46 +34:08:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:59.84 +42:12:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:58.99 +40:37:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:25.80 +40:10:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:59.60 +41:41:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:51.76 +34:12:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:23.98 +38:09:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:18.56 +40:09:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:38.52 +42:15:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:55.09 +40:06:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:00.51 +33:49:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:41.25 +35:46:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:15.67 +37:37:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:17.81 +33:50:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:35.94 +34:50:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:36.83 +35:29:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:23.66 +37:26:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:27.67 +35:29:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:15.22 +37:58:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:24.21 +41:09:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:41.02 +36:01:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:45.83 +36:52:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:51.65 +41:55:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:47.01 +35:30:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:19.48 +38:29:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:38.69 +39:02:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:04.03 +40:34:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:11.41 +40:12:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:13.43 +39:08:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:33.10 +36:29:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:02.51 +37:20:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:07.31 +41:15:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:24.46 +40:48:60.0 -- 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)
19:04:26.08 +40:57:26.3 -- not a known variable star
19:06:43.66 +38:19:04.0 -- not a known variable star
19:08:54.96 +35:55:50.1 -- a known variable star
19:13:13.44 +34:34:38.1 -- not a known variable star
19:24:51.67 +34:41:28.0 -- not a known variable star
19:27:51.60 +39:46:14.6 -- not a known variable star
19:28:15.40 +38:17:60.0 -- a known variable star
19:32:05.46 +34:08:21.6 -- not a known variable star
19:32:59.84 +42:12:10.6 -- not a known variable star
19:35:58.99 +40:37:30.3 -- a known variable star
19:36:25.80 +40:10:57.4 -- a known variable star
19:37:59.60 +41:41:08.3 -- not a known variable star
19:39:51.76 +34:12:15.6 -- not a known variable star
19:40:23.98 +38:09:00.0 -- not a known variable star
19:41:18.56 +40:09:36.8 -- not a known variable star
19:41:38.52 +42:15:45.4 -- a known variable star
19:43:55.09 +40:06:41.7 -- a known variable star
19:44:00.51 +33:49:36.6 -- a known variable star
19:46:41.25 +35:46:36.1 -- not a known variable star
19:47:15.67 +37:37:13.2 -- a known variable star
19:49:17.81 +33:50:35.7 -- not a known variable star
19:49:35.94 +34:50:59.1 -- not a known variable star
19:52:36.83 +35:29:58.0 -- not a known variable star
19:53:23.66 +37:26:33.4 -- a known variable star
19:54:27.67 +35:29:17.1 -- not a known variable star
19:55:15.22 +37:58:47.3 -- a known variable star
19:57:24.21 +41:09:40.0 -- not a known variable star
19:57:41.02 +36:01:16.8 -- not a known variable star
19:57:45.83 +36:52:44.0 -- a known variable star
19:57:51.65 +41:55:01.5 -- not a known variable star
19:58:47.01 +35:30:44.9 -- not a known variable star
19:59:19.48 +38:29:24.0 -- not a known variable star
19:59:38.69 +39:02:21.0 -- not a known variable star
20:01:04.03 +40:34:52.4 -- not a known variable star
20:01:11.41 +40:12:29.3 -- not a known variable star
20:01:13.43 +39:08:56.1 -- not a known variable star
20:01:33.10 +36:29:01.4 -- not a known variable star
20:02:02.51 +37:20:38.6 -- a known variable star
20:07:07.31 +41:15:00.4 -- not a known variable star
20:07:24.46 +40:48:60.0 -- not a known variable star
Found 28 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
40 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:04:26.08 +40:57:26.3
19:06:43.66 +38:19:04.0
19:08:54.96 +35:55:50.1
19:13:13.44 +34:34:38.1
19:24:51.67 +34:41:28.0
19:27:51.60 +39:46:14.6
19:28:15.40 +38:17:60.0
19:32:05.46 +34:08:21.6
19:32:59.84 +42:12:10.6
19:35:58.99 +40:37:30.3
19:36:25.80 +40:10:57.4
19:37:59.60 +41:41:08.3
19:39:51.76 +34:12:15.6
19:40:23.98 +38:09:00.0
19:41:18.56 +40:09:36.8
19:41:38.52 +42:15:45.4
19:43:55.09 +40:06:41.7
19:44:00.51 +33:49:36.6
19:46:41.25 +35:46:36.1
19:47:15.67 +37:37:13.2
19:49:17.81 +33:50:35.7
19:49:35.94 +34:50:59.1
19:52:36.83 +35:29:58.0
19:53:23.66 +37:26:33.4
19:54:27.67 +35:29:17.1
19:55:15.22 +37:58:47.3
19:57:24.21 +41:09:40.0
19:57:41.02 +36:01:16.8
19:57:45.83 +36:52:44.0
19:57:51.65 +41:55:01.5
19:58:47.01 +35:30:44.9
19:59:19.48 +38:29:24.0
19:59:38.69 +39:02:21.0
20:01:04.03 +40:34:52.4
20:01:11.41 +40:12:29.3
20:01:13.43 +39:08:56.1
20:01:33.10 +36:29:01.4
20:02:02.51 +37:20:38.6
20:07:07.31 +41:15:00.4
20:07:24.46 +40:48:60.0
20:02:26.24 +36:42:12.4
19:43:59.69 +39:33:55.7
19:07:17.76 +40:23:25.7
19:32:42.65 +34:20:49.7
19:02:02.96 +41:04:39.1
19:49:47.65 +34:58:34.9
19:55:17.12 +33:59:48.1
19:06:05.32 +41:49:18.6
19:14:54.97 +41:00:12.2
19:36:52.50 +41:25:30.9
19:37:12.22 +38:48:08.1
19:44:05.81 +35:59:03.6
19:57:01.90 +40:11:22.9
19:56:46.53 +37:12:06.5
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461126.89458705 -observatory 500
22:47:07.43 -08:14:39.3 Mercury (0.6mag)
01:35:49.89 +09:18:37.2 Venus (-3.9mag)
23:21:44.75 -05:16:14.0 Mars (1.2mag)
07:05:55.04 +22:56:30.6 Jupiter (-2.2mag)
00:20:16.81 -00:07:18.5 Saturn (0.9mag)
03:43:57.48 +19:35:17.3 Uranus (5.8mag)
00:08:10.78 -00:32:18.2 Neptune (7.8mag)
20:32:32.67 -22:53:03.9 Pluto (14.5mag)
07:58:51.40 +24:09:55.3 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Mar 27 05:28 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461126.89458705:
07:05:49.07 +22:56:43.8 Io (5.6mag)
07:05:53.42 +22:56:30.3 Europa (5.8mag)
07:05:43.69 +22:56:45.2 Ganymede (5.2mag)
07:06:11.16 +22:56:09.9 Callisto (6.5mag)
07:09:52.55 +22:54:25.3 Himalia (15.2mag)
07:05:58.40 +22:56:22.4 Thebe (16.1mag)
07:09:35.88 +23:20:17.8 Elara (17.2mag)
07:03:28.28 +23:46:48.4 Pasiphae (17.3mag)
07:14:36.95 +22:52:03.6 Carme (18.4mag)
00:20:28.56 -00:07:15.7 Titan (8.8mag)
00:20:16.92 -00:07:03.2 Rhea (10.1mag)
00:20:38.13 -00:05:06.7 Iapetus (11.5mag)
00:20:18.45 -00:06:54.6 Hyperion (14.8mag)
00:22:07.36 +00:03:25.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 27 05:29 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461126.89458705:
13:40:23.06 +01:53:27.7 JWST
18:09:08.40 +32:26:48.2 Chandra
08:53:28.69 -46:14:20.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 27 05:28 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461126.89458705 -observatory 500
18:40:32.28 -27:45:07.6 14.0mag P/2010 H2 (Vales)
04:54:21.32 -70:40:24.6 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:15.44 +31:19:33.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:28.38 +08:10:42.4 17.6mag C/2021 G2 (ATLAS)
23:03:58.92 +28:34:43.9 17.0mag C/2022 E2 (ATLAS)
04:07:13.61 +25:28:48.5 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.86 +31:40:23.7 16.1mag C/2022 QE78 (ATLAS)
08:29:48.79 -02:23:21.2 17.2mag C/2022 R6 (PANSTARRS)
18:56:27.07 +16:50:37.3 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:31.65 -11:46:52.1 17.6mag P/2023 B1 (PANSTARRS)
09:19:27.40 -15:12:02.5 17.5mag C/2023 F3 (ATLAS)
21:30:53.38 +61:55:49.7 17.4mag C/2023 H5 (Lemmon)
19:31:11.33 -03:32:38.5 14.4mag C/2023 R1 (PANSTARRS)
21:40:52.55 +83:28:56.1 17.7mag C/2023 X2 (Lemmon)
06:14:00.24 +63:41:58.6 16.9mag C/2024 A1 (ATLAS)
04:25:37.46 +09:29:26.0 9.6mag C/2024 E1 (Wierzchos)
11:17:26.52 +03:58:47.9 18.0mag C/2024 G2 (ATLAS)
16:29:49.20 +03:10:54.3 17.4mag C/2024 G6 (ATLAS)
20:13:17.57 +10:15:30.8 14.8mag C/2024 J3 (ATLAS)
03:09:40.54 -25:32:54.9 16.4mag C/2024 T5 (ATLAS)
05:01:34.18 +50:37:49.3 17.6mag C/2025 J1 (Borisov)
14:54:43.77 +25:58:39.8 14.5mag C/2025 L1 (ATLAS)
02:56:44.85 -23:24:30.9 17.7mag C/2025 Q3 (ATLAS)
22:37:57.51 +19:26:31.2 11.6mag C/2025 R3 (PANSTARRS)
13:02:32.48 +01:44:24.0 17.6mag C/2025 Y1 (ATLAS)
01:51:01.70 -02:13:39.5 12.4mag C/2026 A1 (MAPS)
23:00:02.63 +32:51:33.3 13.9mag C/2026 B2 (Sun-Gao)
18:04:35.77 -10:37:54.1 13.0mag 10P/Tempel
15:22:41.40 +04:47:13.7 12.3mag 24P/Schaumasse
11:09:22.98 -02:14:01.0 15.6mag 29P/Schwassmann-Wachmann
17:49:42.64 -10:23:38.4 17.5mag 40P/Vaisala
10:42:06.88 -05:54:38.5 16.5mag 43P/Wolf-Harrington
01:18:36.80 +14:04:05.7 17.0mag 47P/Ashbrook-Jackson
06:37:39.65 +41:04:28.7 17.1mag 63P/Wild
23:03:04.91 -13:54:21.7 15.7mag 65P/Gunn
03:13:31.13 +13:56:12.3 15.9mag 76P/West-Kohoutek-Ikemura
00:23:02.08 +04:19:33.1 14.6mag 78P/Gehrels
22:00:30.37 -15:02:27.7 14.5mag 88P/Howell
01:17:08.64 +15:07:09.4 15.2mag 93P/Lovas
04:20:29.98 +31:06:30.5 16.4mag 123P/West-Hartley
08:10:30.65 +47:23:11.4 16.2mag 124P/Mrkos
02:03:37.84 +12:06:45.2 16.4mag 128P/Shoemaker-Holt
02:09:32.99 +11:55:56.6 17.4mag 131P/Mueller
23:48:52.76 +05:40:47.8 12.2mag 141P/Machholz
23:59:08.93 -02:18:37.1 12.3mag 141P-A/Machholz
22:55:47.17 -05:18:03.7 15.3mag 141P-D/Machholz
00:08:04.75 -11:09:39.3 15.4mag 162P/SidingSpring
10:35:19.87 +31:56:01.4 17.6mag 164P/Christensen
06:00:50.25 +24:41:20.1 17.6mag 198P/ODAS
15:24:30.24 -02:29:39.1 17.1mag 210P/Christensen
20:35:32.22 -16:08:02.4 17.2mag 218P/LINEAR
17:05:29.29 -16:05:35.5 16.2mag 235P/LINEAR
04:53:48.24 +32:48:01.1 16.4mag 240P/NEAT
07:31:09.08 -07:31:09.3 17.5mag 242P/Spahr
15:47:58.32 +05:34:57.5 17.6mag 391P/Kowalski
07:28:45.88 +21:12:18.1 17.6mag 450P/LONEOS
05:08:53.22 +46:12:32.4 17.3mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 27 05:28 comets.txt
############################################################
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
-rw-r--r-- 1 apache apache 5.8K Mar 27 05:28 asassn_transients_list.txt
############################################################
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 05:29 tocp_transients_list.txt