This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.25 14:02:11.13 +40:23:22.5
79.66114 70.26966 galactic CVn Second-epoch detections are separated by 1.0" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:11.13 +40:23:22.5 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.13 +40:23:22.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.13 +40:23:22.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.44 14:09:54.48 +38:37:06.3
72.90201 69.98387 galactic Boo Second-epoch detections are separated by 1.2" and 9.9 pix
The object was found in VSX23" Gaia DR3 1485292290451713664
Type: ROT
# Max. Min./Amp. JD0 Period
19.540 G 19.730 G
ATTENTION: measured mag 12.44 is 7.1 mag brighter than the VSX record maximum brightness 19.54 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:09:54.48 +38:37:06.3: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:09:54.48 +38:37:06.3: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1485292290451713664,2461258.7083,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1485292290451713664 20260806.2083 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.43 14:01:18.80 +40:48:21.2
80.93457 70.14794 galactic CVn Second-epoch detections are separated by 1.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:01:18.80 +40:48:21.2 (user input) | T | P | (position from user input) J-Ks=0.779+/-0.027 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:18.80 +40:48:21.2: 13.54 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:18.80 +40:48:21.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.35 14:07:19.92 +40:06:50.7
77.35097 69.62703 galactic Boo Second-epoch detections are separated by 2.8" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:07:19.92 +40:06:50.7 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:19.92 +40:06:50.7: 13.63 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:19.92 +40:06:50.7: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.34 14:01:31.10 +40:50:10.9
80.93470 70.09862 galactic CVn Second-epoch detections are separated by 0.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:01:31.10 +40:50:10.9 (user input) | T | P | (position from user input) J-Ks=0.770+/-0.025 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:31.10 +40:50:10.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:31.10 +40:50:10.9: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.30 14:00:54.52 +40:35:07.4
80.55996 70.34409 galactic CVn Second-epoch detections are separated by 1.2" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:54.52 +40:35:07.4 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.205+/-0.034 (F)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.52 +40:35:07.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.52 +40:35:07.4: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.37 13:58:25.13 +40:28:25.9
81.17878 70.78441 galactic CVn Second-epoch detections are separated by 1.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:25.13 +40:28:25.9 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:25.13 +40:28:25.9: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:25.13 +40:28:25.9: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.36 14:39:51.32 +35:28:25.9
59.54693 65.47952 galactic Boo Second-epoch detections are separated by 2.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:51.32 +35:28:25.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.484+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:51.32 +35:28:25.9: 13.42 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:39:51.32 +35:28:25.9: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.42 14:06:51.00 +39:56:44.0
77.09423 69.79729 galactic CVn Second-epoch detections are separated by 0.4" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:06:51.00 +39:56:44.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.676+/-0.025 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:51.00 +39:56:44.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:51.00 +39:56:44.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.37 14:07:30.82 +40:19:50.8
77.80985 69.47716 galactic Boo Second-epoch detections are separated by 0.6" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:07:30.82 +40:19:50.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.281+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:30.82 +40:19:50.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:30.82 +40:19:50.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.34 14:05:16.19 +40:56:53.3
79.94822 69.46699 galactic CVn Second-epoch detections are separated by 2.1" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:05:16.19 +40:56:53.3 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:05:16.19 +40:56:53.3: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:05:16.19 +40:56:53.3: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.22 14:08:26.71 +39:59:58.0
76.74086 69.51232 galactic Boo Second-epoch detections are separated by 1.7" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:08:26.71 +39:59:58.0 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:08:26.71 +39:59:58.0: 13.31 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:08:26.71 +39:59:58.0: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.22,0.05,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
target 20260806.2083 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
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.34 14:00:54.43 +41:44:27.4
83.18140 69.61589 galactic CVn Second-epoch detections are separated by 2.2" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:54.43 +41:44:27.4 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.43 +41:44:27.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.43 +41:44:27.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.40 13:53:23.16 +36:48:08.0
73.22855 73.72044 galactic CVn Second-epoch detections are separated by 1.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:53:23.16 +36:48:08.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.359+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:23.16 +36:48:08.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:23.16 +36:48:08.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.30 14:07:54.06 +39:47:34.8
76.40619 69.71212 galactic Boo Second-epoch detections are separated by 0.5" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:07:54.06 +39:47:34.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.390+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:54.06 +39:47:34.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:54.06 +39:47:34.8: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.20 14:10:06.82 +38:46:27.4
73.24063 69.87253 galactic Boo Second-epoch detections are separated by 1.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:10:06.82 +38:46:27.4 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:06.82 +38:46:27.4: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:06.82 +38:46:27.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.22 14:02:13.87 +40:30:39.0
79.93236 70.18991 galactic CVn Second-epoch detections are separated by 1.1" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:13.87 +40:30:39.0 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:13.87 +40:30:39.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:13.87 +40:30:39.0: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.22,0.05,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
target 20260806.2083 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
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.21 13:58:06.70 +41:25:34.1
83.47812 70.21754 galactic CVn Second-epoch detections are separated by 2.3" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:06.70 +41:25:34.1 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.547+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:06.70 +41:25:34.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:06.70 +41:25:34.1: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.21,0.05,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
target 20260806.2083 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
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.21 14:02:50.01 +41:25:24.1
81.82241 69.53993 galactic CVn Second-epoch detections are separated by 0.8" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:50.01 +41:25:24.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.427+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:50.01 +41:25:24.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:50.01 +41:25:24.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.21,0.05,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
target 20260806.2083 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
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.11 14:03:06.40 +41:03:40.7
80.91420 69.72379 galactic CVn Second-epoch detections are separated by 1.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:03:06.40 +41:03:40.7 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.027 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:06.40 +41:03:40.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:06.40 +41:03:40.7: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.24 13:56:25.85 +41:52:00.8
85.06462 70.15667 galactic CVn Second-epoch detections are separated by 1.6" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:56:25.85 +41:52:00.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.389+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:25.85 +41:52:00.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:25.85 +41:52:00.8: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.04 14:03:15.62 +40:33:06.9
79.68460 70.00875 galactic CVn Second-epoch detections are separated by 0.8" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:03:15.62 +40:33:06.9 (user input) | T | P | (position from user input) J-Ks=0.299+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:15.62 +40:33:06.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:15.62 +40:33:06.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.13 14:00:27.09 +41:20:29.3
82.45459 69.93796 galactic CVn Second-epoch detections are separated by 1.2" and 9.9 pix
The object was found in VSX 1" Gaia DR3 1498732106410850944
Type: ROT
# Max. Min./Amp. JD0 Period
12.930 G 12.970 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:27.09 +41:20:29.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:27.09 +41:20:29.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1498732106410850944,2461258.7083,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1498732106410850944 20260806.2083 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.96 13:53:15.49 +37:10:34.1
74.39507 73.54047 galactic CVn Second-epoch detections are separated by 0.9" and 10.0 pix
The object was found in VSX 0" Gaia DR3 1495427421134452608
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.760 G F
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:15.49 +37:10:34.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:15.49 +37:10:34.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1495427421134452608,2461258.7083,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1495427421134452608 20260806.2083 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.93 14:01:26.05 +40:30:48.2
80.20955 70.30898 galactic CVn Second-epoch detections are separated by 0.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:01:26.05 +40:30:48.2 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:26.05 +40:30:48.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:26.05 +40:30:48.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 11.93CV 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
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.98 14:40:52.57 +35:24:14.7
59.27844 65.29084 galactic Boo Second-epoch detections are separated by 2.1" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:52.57 +35:24:14.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.384+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:52.57 +35:24:14.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:40:52.57 +35:24:14.7: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.84 14:00:24.23 +40:22:01.0
80.21907 70.55366 galactic CVn Second-epoch detections are separated by 1.0" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:24.23 +40:22:01.0 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.23 +40:22:01.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.23 +40:22:01.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.72 14:00:46.23 +41:05:22.4
81.77394 70.05128 galactic CVn Second-epoch detections are separated by 1.3" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:46.23 +41:05:22.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.334+/-0.026 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:46.23 +41:05:22.4: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:46.23 +41:05:22.4: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.80 14:02:11.25 +40:58:45.6
81.03578 69.91092 galactic CVn Second-epoch detections are separated by 0.8" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:11.25 +40:58:45.6 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.25 +40:58:45.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.25 +40:58:45.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2083 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.64 14:00:45.56 +41:00:42.0
81.59998 70.10185 galactic CVn Second-epoch detections are separated by 1.1" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1498619612627238400 | 14:00:45.49 +41:00:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.649+/-0.025 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:45.56 +41:00:42.0: 12.61 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:45.56 +41:00:42.0: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1498619612627238400,2461258.7083,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1498619612627238400 20260806.2083 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.65 14:02:23.88 +40:59:15.8
80.98381 69.87446 galactic CVn Second-epoch detections are separated by 0.9" and 9.9 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 J210.5994+40.9876 | 14:02:23.88 +40:59:15.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.338+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:23.88 +40:59:15.8: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:23.88 +40:59:15.8: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J210.5994+40.9876,2461258.7083,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J210.5994+40.9876 20260806.2083 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 11.57 14:02:09.56 +40:33:39.3
80.07445 70.17058 galactic CVn Second-epoch detections are separated by 1.0" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1497798140002814208 | 14:02:09.56 +40:33:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.529+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:09.56 +40:33:39.3: 12.51 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:09.56 +40:33:39.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1497798140002814208,2461258.7083,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1497798140002814208 20260806.2083 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2083 2461258.7083 12.47 14:02:07.72 +40:51:05.4
80.76163 69.99830 galactic CVn Second-epoch detections are separated by 1.6" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:07.72 +40:51:05.4 (user input) | T | P | (position from user input) J-Ks=0.839+/-0.028 (M)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:07.72 +40:51:05.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:07.72 +40:51:05.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7083,12.47,0.05,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 20260806.2083 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461178.77788297 18.05.2026 06:39:59.089 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
First image: 2461178.77788297 18.05.2026 06:39:59.089 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Last image: 2461258.70861084 06.08.2026 05:00:13.977 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 2 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4212
Objects passed selection criteria: 4199
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 2658.25
Average stars matched: 2602.75 (97.9122 %)
Memory usage VmPeak: 231260 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 00:08:23 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: 2461178.77788297 18.05.2026 06:39:59.089 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
First image: 2461178.77788297 18.05.2026 06:39:59.089 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Last image: 2461258.70861084 06.08.2026 05:00:13.977 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.01
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22302
Objects passed selection criteria: 22247
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: 15276.8
Average stars matched: 14769.5 (96.6796 %)
Memory usage VmPeak: 248776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 00:09:04 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
SExtractor catalog cache: saved Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.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/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.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: 2461258.70808219
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
Saving wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits to local_wcs_cache/
'wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'local_wcs_cache/wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits'
wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits'
wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (1st reference image)
verification OK: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:56.655 +38:01:04.38 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:53.884 +37:59:56.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:10:56.655 +38:01:04.38
Second-epoch image center 14:10:53.884 +37:59:56.77
Angular distance between the image centers 0.0209 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:50.449 +38:00:39.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:10:56.655 +38:01:04.38
Second-epoch image center 14:10:50.449 +38:00:39.61
Angular distance between the image centers 0.0215 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 14:10:53.884 +37:59:56.77
Second-epoch second image center 14:10:50.449 +38:00:39.61
Angular distance between the image centers 0.01639 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.YWm1CZ2QGH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits &> /tmp/tmp.612Of9Yna6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits &> /tmp/tmp.e48WLkcVfb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits &> /tmp/tmp.lxPg8ij4qB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.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_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Found non-empty wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
The reference image (wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits) and catalog (wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat) found
'wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat' -> 'wcsmag.cat'
Read 5741 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1585 to 223.3271 deg, Dec +32.4728 to +43.2526 deg
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
Tycho-2 catalog search boundaries: RA 202.1585 to 223.3271 deg, Dec 32.4728 to 43.2526 deg
Loaded 4566 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3466 out of 3551 total matches.
Matched with Tycho-2 3551 out of 5741 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.589150
a=0.000000 b=1.000000 c=22.589150
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5741 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1585 to 223.3271 deg, Dec +32.4728 to +43.2526 deg
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
Tycho-2 catalog search boundaries: RA 202.1585 to 223.3271 deg, Dec 32.4728 to 43.2526 deg
Loaded 4566 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3466 out of 3551 total matches.
Matched with Tycho-2 3551 out of 5741 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=6.3)
Read 5807 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1636 to 223.3271 deg, Dec +32.4726 to +43.2409 deg
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
Tycho-2 catalog search boundaries: RA 202.1636 to 223.3271 deg, Dec 32.4726 to 43.2409 deg
Loaded 4561 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3456 out of 3558 total matches.
Matched with Tycho-2 3558 out of 5807 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.4 pix Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
2.4 pix fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
2.4 pix fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Limiting magnitude estimates:
15.3 mag. Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
15.3 mag. Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
12.6 mag. fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
12.2 mag. fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.2 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YWm1CZ2QGH (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=296, bad_region=1278, passed=5741
Got 5741 stars (including 4246 good ones) from the SExtractor catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
util/solve_plate_with_UCAC5 got 5741 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4131 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4131 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4126 stars left (next iteration limit 4538)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=4126 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.327 n_q1=1333 n_q2=759 n_q3=1305 n_q4=729 worst_quadrant_to_overall_ratio=1.093
The image catalog is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.612Of9Yna6 (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Checking if the catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS catalog name: wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=330, bad_region=1342, passed=5807
Got 5807 stars (including 4212 good ones) from the SExtractor catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 5807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 4104 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4101 matched stars entering correct_measured_positions(), 4101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4101 matched stars entering correct_measured_positions(), 4709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 4104 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4101 matched stars entering correct_measured_positions(), 4709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4101 matched stars entering correct_measured_positions(), 4709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4101 stars left (next iteration limit 4511)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits N_match=4101 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.321 n_q1=1298 n_q2=781 n_q3=1275 n_q4=747 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -region wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e48WLkcVfb (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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=46, bad_region=230, passed=1103
Got 1103 stars (including 836 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat
util/solve_plate_with_UCAC5 got 1103 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 809 matched stars entering correct_measured_positions(), 804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 809 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 809 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 809 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 809 stars left (next iteration limit 889)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=809 robust_rms=6.569 arcsec worst_quadrant_rms=8.189 arcsec
SIP_REFIT: SIP order 3 trial: matched=809 robust_rms=0.506 arcsec worst_quadrant_rms=0.633 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=809 robust_rms_before=0.878 arcsec robust_rms_before_corrected=0.393 arcsec robust_rms_after=0.506 arcsec worst_quadrant_rms_before=0.415 worst_quadrant_rms_after=0.633
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.415 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits N_match=809 sigma_overall_arcsec=0.422 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.454 sigma_q4_arcsec=0.410 n_q1=208 n_q2=151 n_q3=288 n_q4=162 worst_quadrant_to_overall_ratio=1.075
The image catalog is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits -region wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lxPg8ij4qB (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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=42, bad_region=222, passed=1121
Got 1121 stars (including 865 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat
util/solve_plate_with_UCAC5 got 1121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 840 matched stars entering correct_measured_positions(), 833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 840 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 840 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 840 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 840 stars left (next iteration limit 924)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=840 robust_rms=6.536 arcsec worst_quadrant_rms=9.482 arcsec
SIP_REFIT: SIP order 3 trial: matched=840 robust_rms=0.510 arcsec worst_quadrant_rms=0.596 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=840 robust_rms_before=0.882 arcsec robust_rms_before_corrected=0.407 arcsec robust_rms_after=0.510 arcsec worst_quadrant_rms_before=0.431 worst_quadrant_rms_after=0.596
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.431 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits N_match=840 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.402 sigma_q4_arcsec=0.362 n_q1=216 n_q2=151 n_q3=304 n_q4=169 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits -region wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits sigma_overall=0.335 worst_q_ratio=1.093
ref2=Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits sigma_overall=0.318 worst_q_ratio=1.120
new1=fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits sigma_overall=0.422 worst_q_ratio=1.075
new2=fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits sigma_overall=0.403 worst_q_ratio=1.079
reference average sigma_overall=0.3265 worst_q_ratio=1.1065
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621_astrometric_residuals.png (4126 matched stars from wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181_astrometric_residuals.png (4101 matched stars from wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172_astrometric_residuals.png (809 matched stars from wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173_astrometric_residuals.png (840 matched stars from wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits'
Preparing the HTML report for the field Boo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Boo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
SExtractor catalog cache: saved Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Creating symlink local_wcs_cache/wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.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_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (1st reference image)
verification OK: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:56.655 +38:01:04.38 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:53.884 +37:59:56.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:10:56.655 +38:01:04.38
Second-epoch image center 14:10:53.884 +37:59:56.77
Angular distance between the image centers 0.0209 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:50.449 +38:00:39.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:10:56.655 +38:01:04.38
Second-epoch image center 14:10:50.449 +38:00:39.61
Angular distance between the image centers 0.0215 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 14:10:53.884 +37:59:56.77
Second-epoch second image center 14:10:50.449 +38:00:39.61
Angular distance between the image centers 0.01639 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.igzykONYOC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits &> /tmp/tmp.o4ZWdomAIS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits &> /tmp/tmp.dZhXko1XIR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits &> /tmp/tmp.GEetJV6p3p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.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_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Found non-empty wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
The reference image (wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits) and catalog (wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat) found
'wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat' -> 'wcsmag.cat'
Read 29344 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1584 to 223.3857 deg, Dec +32.4469 to +43.2802 deg
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
Tycho-2 catalog search boundaries: RA 202.1584 to 223.3857 deg, Dec 32.4469 to 43.2802 deg
Loaded 4602 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3319 out of 3580 total matches.
Matched with Tycho-2 3580 out of 29344 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.475400
a=0.000000 b=1.000000 c=22.475400
From vast_summary.log: estimated ref. image limiting mag.: -7.01
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29344 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1584 to 223.3857 deg, Dec +32.4469 to +43.2802 deg
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
Tycho-2 catalog search boundaries: RA 202.1584 to 223.3857 deg, Dec 32.4469 to 43.2802 deg
Loaded 4602 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3319 out of 3580 total matches.
Matched with Tycho-2 3580 out of 29344 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=4.9)
Read 29317 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1637 to 223.3628 deg, Dec +32.4469 to +43.2481 deg
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
Tycho-2 catalog search boundaries: RA 202.1637 to 223.3628 deg, Dec 32.4469 to 43.2481 deg
Loaded 4588 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3316 out of 3579 total matches.
Matched with Tycho-2 3579 out of 29317 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.2 pix Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
2.2 pix fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
2.1 pix fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Limiting magnitude estimates:
15.5 mag. Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
15.4 mag. Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
12.8 mag. fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
12.8 mag. fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.igzykONYOC (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1045, bad_region=5024, passed=29331
Got 29331 stars (including 23457 good ones) from the SExtractor catalog wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
util/solve_plate_with_UCAC5 got 29331 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 25512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 25512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 25512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4847 stars left (next iteration limit 5331)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=4847 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.330 n_q1=1629 n_q2=900 n_q3=1472 n_q4=846 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.o4ZWdomAIS (6) ############
Parsing command line arguments...
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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Checking if the catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS catalog name: wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1142, bad_region=4900, passed=29301
Got 29301 stars (including 23470 good ones) from the SExtractor catalog wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 29301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 25602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 25602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 25602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits N_match=4852 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.323 n_q1=1581 n_q2=923 n_q3=1462 n_q4=886 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -region wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dZhXko1XIR (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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=125, bad_region=1034, passed=7447
Got 7447 stars (including 6314 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat
util/solve_plate_with_UCAC5 got 7447 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 6679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4820 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 6679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 6679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 4811 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits N_match=4811 sigma_overall_arcsec=0.663 sigma_q1_arcsec=0.702 sigma_q2_arcsec=0.619 sigma_q3_arcsec=0.710 sigma_q4_arcsec=0.580 n_q1=1284 n_q2=964 n_q3=1624 n_q4=939 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits -region wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GEetJV6p3p (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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=129, bad_region=1037, passed=7436
Got 7436 stars (including 6304 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat
util/solve_plate_with_UCAC5 got 7436 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 4810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 6661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4818 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 6661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 6661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 4808 stars left (next iteration limit 5291)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits N_match=4808 sigma_overall_arcsec=0.669 sigma_q1_arcsec=0.676 sigma_q2_arcsec=0.652 sigma_q3_arcsec=0.730 sigma_q4_arcsec=0.568 n_q1=1321 n_q2=921 n_q3=1628 n_q4=938 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits -region wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/wcs_fd_Boo-04-Q2b1x1_2026-08-05_23-59-28_20.00sec_-0.00C_LIGHT_0172.fits
Saving fully-calibrated image wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.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_2026-08-06_CI_Boo-04-Q2b1x1_000513_TTUQ2b1x1_2650938_ts7pp24m/wcs_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173.fits
Preparing the HTML report for the field Boo-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:09:54.48 +38:37:06.3: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.52 +40:35:07.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:19.92 +40:06:50.7: 13.63 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:51.00 +39:56:44.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:25.13 +40:28:25.9: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:14:31.34 +39:15:21.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.13 +40:23:22.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:51.32 +35:28:25.9: 13.42 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:18.80 +40:48:21.2: 13.54 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:31.10 +40:50:10.9: 13.61 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:51.00 +39:56:44.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:14:31.34 +39:15:21.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.13 +40:23:22.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:18.80 +40:48:21.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.52 +40:35:07.4: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:19.92 +40:06:50.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:09:54.48 +38:37:06.3: 13.42 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:39:51.32 +35:28:25.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:25.13 +40:28:25.9: 13.53 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:31.10 +40:50:10.9: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 14:06:51.00 +39:56:44.0: ref_mag=13.41 +/- 0.02 new_mean_mag=12.4187 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 14:02:11.13 +40:23:22.5: ref_mag=13.35 +/- 0.02 new_mean_mag=12.2414 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 14:01:18.80 +40:48:21.2: ref_mag=13.53 +/- 0.02 new_mean_mag=12.4286 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 14:00:54.52 +40:35:07.4: ref_mag=13.43 +/- 0.02 new_mean_mag=12.2843 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 14:07:19.92 +40:06:50.7: ref_mag=13.67 +/- 0.03 new_mean_mag=12.3273 delta=1.34 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:14:31.34 +39:15:21.0: ref_mag=12.87 +/- 0.02 new_mean_mag=12.2381 delta=0.64 (need > 0.90)
Forced photometry filter KEPT candidate at 13:58:25.13 +40:28:25.9: ref_mag=13.49 +/- 0.02 new_mean_mag=12.3173 delta=1.18 (need > 0.90)
Forced photometry filter KEPT candidate at 14:09:54.48 +38:37:06.3: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4080 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 14:39:51.32 +35:28:25.9: ref_mag=13.47 +/- 0.03 new_mean_mag=12.3068 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 14:01:31.10 +40:50:10.9: ref_mag=13.57 +/- 0.02 new_mean_mag=12.3585 delta=1.21 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:30.82 +40:19:50.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:30.82 +40:19:50.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 14:07:30.82 +40:19:50.8: ref_mag=13.38 +/- 0.02 new_mean_mag=12.2919 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:05:16.19 +40:56:53.3: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:05:16.19 +40:56:53.3: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 14:05:16.19 +40:56:53.3: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3405 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:08:26.71 +39:59:58.0: 13.31 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:08:26.71 +39:59:58.0: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 14:08:26.71 +39:59:58.0: ref_mag=13.32 +/- 0.02 new_mean_mag=12.1947 delta=1.13 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.43 +41:44:27.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:23.16 +36:48:08.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.43 +41:44:27.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 14:00:54.43 +41:44:27.4: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3164 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:23.16 +36:48:08.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 13:53:23.16 +36:48:08.0: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3997 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:54.06 +39:47:34.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:06.82 +38:46:27.4: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:54.06 +39:47:34.8: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 14:07:54.06 +39:47:34.8: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2854 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:13.87 +40:30:39.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:06.70 +41:25:34.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:50.01 +41:25:24.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:06.82 +38:46:27.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 14:10:06.82 +38:46:27.4: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1782 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:13.87 +40:30:39.0: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 14:02:13.87 +40:30:39.0: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2081 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:06.70 +41:25:34.1: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 13:58:06.70 +41:25:34.1: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1917 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:50.01 +41:25:24.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 14:02:50.01 +41:25:24.1: ref_mag=13.21 +/- 0.02 new_mean_mag=12.1799 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:06.40 +41:03:40.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:06.40 +41:03:40.7: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 14:03:06.40 +41:03:40.7: ref_mag=13.17 +/- 0.02 new_mean_mag=12.0659 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:25.85 +41:52:00.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:25.85 +41:52:00.8: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 13:56:25.85 +41:52:00.8: ref_mag=13.12 +/- 0.02 new_mean_mag=12.2122 delta=0.91 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:15.62 +40:33:06.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:15.62 +40:33:06.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 14:03:15.62 +40:33:06.9: ref_mag=13.05 +/- 0.02 new_mean_mag=11.9815 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:27.09 +41:20:29.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:15.49 +37:10:34.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:15.49 +37:10:34.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:27.09 +41:20:29.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 13:53:15.49 +37:10:34.1: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9641 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 14:00:27.09 +41:20:29.3: ref_mag=13.04 +/- 0.02 new_mean_mag=12.1136 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:26.05 +40:30:48.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:52.57 +35:24:14.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:26.05 +40:30:48.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 14:01:26.05 +40:30:48.2: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9308 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:40:52.57 +35:24:14.7: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 14:40:52.57 +35:24:14.7: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9783 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.23 +40:22:01.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:18.19 +41:12:45.6: 12.71 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:46.23 +41:05:22.4: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.23 +40:22:01.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:24.23 +40:22:01.0: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7990 delta=0.90 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:18.19 +41:12:45.6: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter REJECTED candidate at 14:00:18.19 +41:12:45.6: ref_mag=12.72 +/- 0.01 new_mean_mag=11.8323 delta=0.89 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:46.23 +41:05:22.4: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:46.23 +41:05:22.4: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7243 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.25 +40:58:45.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:23.88 +40:59:15.8: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:45.56 +41:00:42.0: 12.61 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:09.56 +40:33:39.3: 12.51 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:07.72 +40:51:05.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.25 +40:58:45.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 14:02:11.25 +40:58:45.6: ref_mag=12.71 +/- 0.01 new_mean_mag=11.8005 delta=0.91 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:45.56 +41:00:42.0: 12.57 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:23.88 +40:59:15.8: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:45.56 +41:00:42.0: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6307 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 14:02:23.88 +40:59:15.8: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6499 delta=0.90 (need > 0.90)
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:09.56 +40:33:39.3: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry on wcs_Boo-04-Q2b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:07.72 +40:51:05.4: 13.59 +/- 0.04 detection
Forced photometry filter KEPT candidate at 14:02:09.56 +40:33:39.3: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5756 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 14:02:07.72 +40:51:05.4: ref_mag=13.65 +/- 0.03 new_mean_mag=12.4640 delta=1.19 (need > 0.90)
Adding exclusion_list_local.txt__out03618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26919.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 47s
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: 18s
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Considering the candidate 31984_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
The candidate 31984_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173 did not pass the final checks
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Considering the candidate 07916_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07916_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 13058_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 13058_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06707_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06707_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 08760_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 08760_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06607_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06607_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07350_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07350_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07628_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07628_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 22805_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 22805_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 09219_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 09219_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 08140_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 08140_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06358_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06358_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 09090_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 09090_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 04075_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 04075_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 20908_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 20908_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 15766_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
The candidate 15766_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173 did not pass the final checks
**** FOUND 13:50:44.19 +37:37:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09611_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 09611_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 12574_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 12574_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07566_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07566_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 04876_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 04876_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 04956_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 04956_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06043_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06043_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 03618_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 03618_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07455_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07455_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 05188_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 05188_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 17135_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 17135_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07540_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07540_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 26919_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 26919_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07934_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07934_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05574_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
The candidate 05574_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173 did not pass the final checks
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Considering the candidate 05896_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 05896_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06237_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06237_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06125_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06125_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06216_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06216_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 07400_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 07400_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
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Considering the candidate 06587_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
Preparing report for the candidate 06587_fd_Boo-04-Q2b1x1_2026-08-06_00-00-13_20.00sec_-0.00C_LIGHT_0173
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 67s
Prepared the HTML report for the field Boo-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:56:25.85 +41:52:00.8
14:00:54.43 +41:44:27.4
13:58:06.70 +41:25:34.1
14:02:50.01 +41:25:24.1
14:00:27.09 +41:20:29.3
14:00:46.23 +41:05:22.4
14:03:06.40 +41:03:40.7
14:00:45.56 +41:00:42.0
14:02:23.88 +40:59:15.8
14:02:11.25 +40:58:45.6
14:05:16.19 +40:56:53.3
14:02:07.72 +40:51:05.4
14:01:31.10 +40:50:10.9
14:01:18.80 +40:48:21.2
14:00:54.52 +40:35:07.4
14:02:09.56 +40:33:39.3
14:03:15.62 +40:33:06.9
14:01:26.05 +40:30:48.2
14:02:13.87 +40:30:39.0
13:58:25.13 +40:28:25.9
14:02:11.13 +40:23:22.5
14:00:24.23 +40:22:01.0
14:07:30.82 +40:19:50.8
14:07:19.92 +40:06:50.7
14:08:26.71 +39:59:58.0
14:06:51.00 +39:56:44.0
14:07:54.06 +39:47:34.8
14:10:06.82 +38:46:27.4
14:09:54.48 +38:37:06.3
13:53:15.49 +37:10:34.1
13:53:23.16 +36:48:08.0
14:39:51.32 +35:28:25.9
14:40:52.57 +35:24:14.7
########### Completed Boo-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
14:02:11.13 +40:23:22.5
14:09:54.48 +38:37:06.3
14:01:18.80 +40:48:21.2
14:07:19.92 +40:06:50.7
14:01:31.10 +40:50:10.9
14:00:54.52 +40:35:07.4
13:58:25.13 +40:28:25.9
14:39:51.32 +35:28:25.9
14:06:51.00 +39:56:44.0
14:07:30.82 +40:19:50.8
14:05:16.19 +40:56:53.3
14:08:26.71 +39:59:58.0
14:00:54.43 +41:44:27.4
13:53:23.16 +36:48:08.0
14:07:54.06 +39:47:34.8
14:10:06.82 +38:46:27.4
14:02:13.87 +40:30:39.0
13:58:06.70 +41:25:34.1
14:02:50.01 +41:25:24.1
14:03:06.40 +41:03:40.7
13:56:25.85 +41:52:00.8
14:03:15.62 +40:33:06.9
14:00:27.09 +41:20:29.3
13:53:15.49 +37:10:34.1
14:01:26.05 +40:30:48.2
14:40:52.57 +35:24:14.7
14:00:24.23 +40:22:01.0
14:00:46.23 +41:05:22.4
14:02:11.25 +40:58:45.6
14:00:45.56 +41:00:42.0
14:02:23.88 +40:59:15.8
14:02:09.56 +40:33:39.3
14:02:07.72 +40:51:05.4
###################################################################################
14:02:11.13 +40:23:22.5 -- not an asteroid (will add it to exclusion list)
14:09:54.48 +38:37:06.3 -- not an asteroid (will add it to exclusion list)
14:01:18.80 +40:48:21.2 -- not an asteroid (will add it to exclusion list)
14:07:19.92 +40:06:50.7 -- not an asteroid (will add it to exclusion list)
14:01:31.10 +40:50:10.9 -- not an asteroid (will add it to exclusion list)
14:00:54.52 +40:35:07.4 -- not an asteroid (will add it to exclusion list)
13:58:25.13 +40:28:25.9 -- not an asteroid (will add it to exclusion list)
14:39:51.32 +35:28:25.9 -- not an asteroid (will add it to exclusion list)
14:06:51.00 +39:56:44.0 -- not an asteroid (will add it to exclusion list)
14:07:30.82 +40:19:50.8 -- not an asteroid (will add it to exclusion list)
14:05:16.19 +40:56:53.3 -- not an asteroid (will add it to exclusion list)
14:08:26.71 +39:59:58.0 -- not an asteroid (will add it to exclusion list)
14:00:54.43 +41:44:27.4 -- not an asteroid (will add it to exclusion list)
13:53:23.16 +36:48:08.0 -- not an asteroid (will add it to exclusion list)
14:07:54.06 +39:47:34.8 -- not an asteroid (will add it to exclusion list)
14:10:06.82 +38:46:27.4 -- not an asteroid (will add it to exclusion list)
14:02:13.87 +40:30:39.0 -- not an asteroid (will add it to exclusion list)
13:58:06.70 +41:25:34.1 -- not an asteroid (will add it to exclusion list)
14:02:50.01 +41:25:24.1 -- not an asteroid (will add it to exclusion list)
14:03:06.40 +41:03:40.7 -- not an asteroid (will add it to exclusion list)
13:56:25.85 +41:52:00.8 -- not an asteroid (will add it to exclusion list)
14:03:15.62 +40:33:06.9 -- not an asteroid (will add it to exclusion list)
14:00:27.09 +41:20:29.3 -- not an asteroid (will add it to exclusion list)
13:53:15.49 +37:10:34.1 -- not an asteroid (will add it to exclusion list)
14:01:26.05 +40:30:48.2 -- not an asteroid (will add it to exclusion list)
14:40:52.57 +35:24:14.7 -- not an asteroid (will add it to exclusion list)
14:00:24.23 +40:22:01.0 -- not an asteroid (will add it to exclusion list)
14:00:46.23 +41:05:22.4 -- not an asteroid (will add it to exclusion list)
14:02:11.25 +40:58:45.6 -- not an asteroid (will add it to exclusion list)
14:00:45.56 +41:00:42.0 -- not an asteroid (will add it to exclusion list)
14:02:23.88 +40:59:15.8 -- not an asteroid (will add it to exclusion list)
14:02:09.56 +40:33:39.3 -- not an asteroid (will add it to exclusion list)
14:02:07.72 +40:51:05.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
13:53:15.49 +37:10:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:53:23.16 +36:48:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:56:25.85 +41:52:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:06.70 +41:25:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:25.13 +40:28:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:24.23 +40:22:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:27.09 +41:20:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:45.56 +41:00:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:46.23 +41:05:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:54.43 +41:44:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:54.52 +40:35:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:18.80 +40:48:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:26.05 +40:30:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:31.10 +40:50:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:07.72 +40:51:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:09.56 +40:33:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:11.13 +40:23:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:11.25 +40:58:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:13.87 +40:30:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:23.88 +40:59:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:50.01 +41:25:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:06.40 +41:03:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:15.62 +40:33:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:05:16.19 +40:56:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:06:51.00 +39:56:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:19.92 +40:06:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:30.82 +40:19:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:54.06 +39:47:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:26.71 +39:59:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:54.48 +38:37:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:06.82 +38:46:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:51.32 +35:28:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:52.57 +35:24:14.7 -- 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)
13:53:15.49 +37:10:34.1 -- a known variable star
13:53:23.16 +36:48:08.0 -- not a known variable star
13:56:25.85 +41:52:00.8 -- not a known variable star
13:58:06.70 +41:25:34.1 -- not a known variable star
13:58:25.13 +40:28:25.9 -- not a known variable star
14:00:24.23 +40:22:01.0 -- not a known variable star
14:00:27.09 +41:20:29.3 -- a known variable star
14:00:45.56 +41:00:42.0 -- not a known variable star
14:00:46.23 +41:05:22.4 -- not a known variable star
14:00:54.43 +41:44:27.4 -- not a known variable star
14:00:54.52 +40:35:07.4 -- not a known variable star
14:01:18.80 +40:48:21.2 -- not a known variable star
14:01:26.05 +40:30:48.2 -- not a known variable star
14:01:31.10 +40:50:10.9 -- not a known variable star
14:02:07.72 +40:51:05.4 -- not a known variable star
14:02:09.56 +40:33:39.3 -- not a known variable star
14:02:11.13 +40:23:22.5 -- not a known variable star
14:02:11.25 +40:58:45.6 -- not a known variable star
14:02:13.87 +40:30:39.0 -- not a known variable star
14:02:23.88 +40:59:15.8 -- not a known variable star
14:02:50.01 +41:25:24.1 -- not a known variable star
14:03:06.40 +41:03:40.7 -- not a known variable star
14:03:15.62 +40:33:06.9 -- not a known variable star
14:05:16.19 +40:56:53.3 -- not a known variable star
14:06:51.00 +39:56:44.0 -- not a known variable star
14:07:19.92 +40:06:50.7 -- not a known variable star
14:07:30.82 +40:19:50.8 -- not a known variable star
14:07:54.06 +39:47:34.8 -- not a known variable star
14:08:26.71 +39:59:58.0 -- not a known variable star
14:09:54.48 +38:37:06.3 -- a known variable star
14:10:06.82 +38:46:27.4 -- not a known variable star
14:39:51.32 +35:28:25.9 -- not a known variable star
14:40:52.57 +35:24:14.7 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
33 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
13:53:15.49 +37:10:34.1
13:53:23.16 +36:48:08.0
13:56:25.85 +41:52:00.8
13:58:06.70 +41:25:34.1
13:58:25.13 +40:28:25.9
14:00:24.23 +40:22:01.0
14:00:27.09 +41:20:29.3
14:00:45.56 +41:00:42.0
14:00:46.23 +41:05:22.4
14:00:54.43 +41:44:27.4
14:00:54.52 +40:35:07.4
14:01:18.80 +40:48:21.2
14:01:26.05 +40:30:48.2
14:01:31.10 +40:50:10.9
14:02:07.72 +40:51:05.4
14:02:09.56 +40:33:39.3
14:02:11.13 +40:23:22.5
14:02:11.25 +40:58:45.6
14:02:13.87 +40:30:39.0
14:02:23.88 +40:59:15.8
14:02:50.01 +41:25:24.1
14:03:06.40 +41:03:40.7
14:03:15.62 +40:33:06.9
14:05:16.19 +40:56:53.3
14:06:51.00 +39:56:44.0
14:07:19.92 +40:06:50.7
14:07:30.82 +40:19:50.8
14:07:54.06 +39:47:34.8
14:08:26.71 +39:59:58.0
14:09:54.48 +38:37:06.3
14:10:06.82 +38:46:27.4
14:39:51.32 +35:28:25.9
14:40:52.57 +35:24:14.7
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.70808219 -observatory V36
07:45:33.93 +20:23:14.4 Mercury (-0.3mag)
11:55:38.64 -00:03:40.1 Venus (-4.3mag)
05:43:24.37 +23:32:38.2 Mars (1.3mag)
08:41:07.50 +18:48:00.5 Jupiter (-1.8mag)
00:56:33.01 +03:16:47.5 Saturn (0.6mag)
04:11:29.63 +20:56:20.4 Uranus (5.8mag)
00:16:12.83 +00:13:59.1 Neptune (7.7mag)
20:28:20.07 -23:29:24.0 Pluto (14.4mag)
02:46:13.29 +20:31:28.5 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 00:08 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.70808219:
08:41:14.53 +18:47:30.6 Io (6.0mag)
08:41:04.41 +18:48:14.2 Europa (6.3mag)
08:41:03.88 +18:48:19.9 Ganymede (5.6mag)
08:40:53.66 +18:49:02.7 Callisto (6.7mag)
08:38:43.40 +18:46:09.9 Himalia (15.7mag)
08:41:05.82 +18:48:08.5 Thebe (16.6mag)
08:38:14.03 +18:45:05.4 Elara (17.7mag)
08:45:13.40 +18:28:25.5 Pasiphae (17.9mag)
08:44:26.36 +18:57:50.7 Carme (19.0mag)
00:56:30.83 +03:17:14.4 Titan (8.4mag)
00:56:27.30 +03:16:51.4 Rhea (9.7mag)
00:56:36.61 +03:15:09.6 Iapetus (11.1mag)
00:56:19.63 +03:17:01.9 Hyperion (14.4mag)
00:55:58.06 +03:10:14.3 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 00:08 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.70808219:
18:55:36.97 -24:03:55.2 JWST
17:13:13.41 +42:04:21.2 Chandra
09:20:26.70 -52:45:05.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 00:08 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.70808219 -observatory V36
03:11:22.41 +17:12:22.9 17.7mag P/1996 R2 (Lagerkvist)
18:02:24.82 -34:38:24.2 14.0mag P/2010 H2 (Vales)
06:51:54.27 -68:49:37.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:16.83 +32:57:04.3 17.7mag C/2017 K2 (PANSTARRS)
03:37:40.63 +36:43:30.5 16.7mag P/2021 N1 (ZTF)
22:40:17.39 +31:33:58.7 17.3mag C/2022 E2 (ATLAS)
06:41:28.07 +26:34:32.2 16.8mag C/2022 N2 (PANSTARRS)
10:19:42.22 +28:33:37.3 17.0mag C/2022 QE78 (ATLAS)
09:27:30.53 +05:17:43.2 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.07 -12:12:26.7 17.9mag P/2023 B1 (PANSTARRS)
21:13:26.17 +66:13:59.9 17.9mag C/2023 H5 (Lemmon)
15:49:55.19 -12:44:51.8 14.3mag C/2023 R1 (PANSTARRS)
08:05:49.23 +31:15:18.5 15.2mag C/2024 E1 (Wierzchos)
15:07:17.92 +15:36:58.8 17.7mag C/2024 G6 (ATLAS)
19:05:41.49 +42:57:38.8 13.7mag C/2024 J3 (ATLAS)
21:13:41.34 +49:04:39.1 17.6mag C/2024 R4 (PANSTARRS)
05:13:30.66 -12:59:39.0 15.5mag C/2024 T5 (ATLAS)
06:54:54.32 +24:30:37.8 17.9mag C/2025 J1 (Borisov)
07:29:56.52 -15:51:53.9 17.7mag C/2025 R3 (PANSTARRS)
10:30:06.32 +21:01:55.5 17.3mag C/2025 V2 (Rankin)
12:56:55.91 +02:28:58.9 17.0mag C/2025 Y1 (ATLAS)
16:03:42.48 +78:01:11.6 16.8mag C/2026 A2 (Bok)
03:06:42.63 +46:08:41.5 17.1mag C/2026 B2 (Sun-Gao)
11:45:08.09 +08:19:51.2 17.3mag A/2026 E1
21:56:06.03 -26:26:59.0 6.9mag 10P/Tempel
11:27:45.48 -03:16:32.0 16.2mag 29P/Schwassmann-Wachmann
04:36:44.25 +32:15:38.2 18.0mag 47P/Ashbrook-Jackson
11:03:34.60 +05:18:06.1 17.2mag 63P/Wild
00:54:17.94 -05:22:40.8 15.4mag 65P/Gunn
05:30:57.92 +20:43:47.0 13.7mag 78P/Gehrels
20:39:48.40 -23:17:25.1 17.8mag 84P/Giclas
02:58:42.50 +13:32:18.3 16.7mag 88P/Howell
07:50:43.30 +27:55:49.8 16.1mag 93P/Lovas
04:00:41.29 +16:05:25.7 17.6mag 112P/Urata-Niijima
05:49:48.95 +30:30:58.1 16.3mag 114P/Wiseman-Skiff
09:13:42.57 +26:59:19.1 15.0mag 123P/West-Hartley
11:39:42.15 -09:29:32.2 17.1mag 124P/Mrkos
05:33:34.41 +21:11:10.6 16.1mag 128P/Shoemaker-Holt
06:25:03.40 +18:59:48.7 17.9mag 131P/Mueller
00:03:41.97 +03:25:21.9 17.6mag 139P/Vaisala-Oterma
03:21:34.30 -19:44:56.2 14.0mag 161P/Hartley-IRAS
07:09:10.99 +37:41:19.6 15.8mag 162P/SidingSpring
15:50:12.54 +39:28:48.5 12.3mag 169P/NEAT
02:39:16.58 +09:28:30.3 17.6mag 220P/McNaught
16:40:34.89 -09:56:36.1 17.6mag 235P/LINEAR
20:23:44.73 -52:50:55.5 17.8mag 259P/Garradd
03:16:14.29 +24:18:46.1 15.4mag 260P/McNaught
06:59:17.28 +37:45:17.8 17.3mag 295P/LINEAR
15:09:50.70 +03:21:38.3 17.7mag 391P/Kowalski
08:59:02.79 +18:28:29.3 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 00:08 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 00:08 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 00:08 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
18:14:11.533 +25:31:50.45 AT 2026vkg 2026-07-16.29 20.95
22:50:03.729 +40:38:42.44 AT 2026vkf 2026-07-20.53 20.32
-rw-r--r-- 1 apache apache 87K Aug 6 00:08 tns_transients_list.txt
