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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM
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 06.2084 2461258.7083 11.45 13:57:27.32 +41:51:47.1
84.67771 70.01871 galactic CVn Second-epoch detections are separated by 1.6" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1498905004614111744
Type: ROT
# Max. Min./Amp. JD0 Period
12.210 G 12.230 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:57:27.32 +41:51:47.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:57:27.32 +41:51:47.1: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 1498905004614111744,2461258.7083,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1498905004614111744 20260806.2084 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.74 14:00:49.23 +42:18:23.7
84.42886 69.25778 galactic CVn Second-epoch detections are separated by 1.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1498835872820674816 | 14:00:49.35 +42:18:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:49.23 +42:18:23.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:49.23 +42:18:23.7: 12.63 +/- 0.02 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
Gaia DR3 1498835872820674816,2461258.7083,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1498835872820674816 20260806.2084 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.72 14:02:11.27 +40:58:45.7
81.03573 69.91085 galactic CVn Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:11.27 +40:58:45.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.27 +40:58:45.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.27 +40:58:45.7: 12.72 +/- 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,2461258.7083,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 11.68 14:00:50.53 +40:42:53.0
80.88551 70.27442 galactic CVn Second-epoch detections are separated by 0.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:50.53 +40:42:53.0 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:50.53 +40:42:53.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:50.53 +40:42:53.0: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 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,2461258.7083,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.00 13:57:54.07 +42:10:37.3
85.18831 69.74563 galactic CVn Second-epoch detections are separated by 0.8" and 6.7 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 | 13:57:54.07 +42:10:37.3 (user input) | T | P | (position from user input) J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:57:54.07 +42:10:37.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:57:54.07 +42:10:37.3: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461258.7083,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.27 14:06:43.22 +41:28:46.4
80.68702 68.93035 galactic CVn Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:06:43.22 +41:28:46.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.412+/-0.026 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:43.22 +41:28:46.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:43.22 +41:28:46.4: 13.30 +/- 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,2461258.7083,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.40 14:10:16.59 +39:21:29.9
74.65170 69.55201 galactic Boo Second-epoch detections are separated by 2.1" and 6.8 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 | 14:10:16.59 +39:21:29.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.395+/-0.038 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:16.59 +39:21:29.9: 13.50 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:16.59 +39:21:29.9: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.30 13:59:51.83 +41:25:51.9
82.86141 69.96497 galactic CVn Second-epoch detections are separated by 1.2" and 6.7 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 | 13:59:51.83 +41:25:51.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.618+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:59:51.83 +41:25:51.9: 13.52 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:59:51.83 +41:25:51.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 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-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.30 14:08:32.46 +40:00:56.6
76.75128 69.48806 galactic Boo Second-epoch detections are separated by 2.7" and 7.1 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 | 14:08:32.46 +40:00:56.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.510+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:08:32.46 +40:00:56.6: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:08:32.46 +40:00:56.6: 13.38 +/- 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-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.23 14:00:54.47 +40:35:06.8
80.55986 70.34432 galactic CVn Second-epoch detections are separated by 2.4" and 6.7 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 | 14:00:54.47 +40:35:06.8 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.47 +40:35:06.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.47 +40:35:06.8: 13.40 +/- 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,2461258.7083,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.40 14:46:06.28 +34:11:34.1
56.02839 64.44535 galactic Boo Second-epoch detections are separated by 2.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J221.5416+34.1948 | 14:46:06.28 +34:11:34.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:06.28 +34:11:34.1: 13.46 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:46:06.28 +34:11:34.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
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 J221.5416+34.1948,2461258.7083,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J221.5416+34.1948 20260806.2084 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 06.2084 2461258.7083 12.24 14:07:30.81 +40:19:51.4
77.81029 69.47710 galactic Boo Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:07:30.81 +40:19:51.4 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:30.81 +40:19:51.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:30.81 +40:19:51.4: 13.40 +/- 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
target,2461258.7083,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.38 14:12:44.99 +37:28:35.1
69.18467 70.00890 galactic Boo Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:12:44.99 +37:28:35.1 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:12:44.99 +37:28:35.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:12:44.99 +37:28:35.1: 13.42 +/- 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,2461258.7083,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.18 14:00:10.17 +41:49:26.7
83.61999 69.66629 galactic CVn Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:10.17 +41:49:26.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.304+/-0.029 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:10.17 +41:49:26.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:10.17 +41:49:26.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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,2461258.7083,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.09 13:58:40.74 +41:35:23.9
83.63620 70.02983 galactic CVn Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:40.74 +41:35:23.9 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.302+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:40.74 +41:35:23.9: 13.28 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:40.74 +41:35:23.9: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461258.7083,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.29 14:37:31.58 +34:15:38.0
56.86769 66.18487 galactic Boo Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:37:31.58 +34:15:38.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:31.58 +34:15:38.0: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:37:31.58 +34:15:38.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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,2461258.7083,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.11 14:43:45.02 +33:35:07.3
54.77440 65.01206 galactic Boo Second-epoch detections are separated by 0.5" and 6.7 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 | 14:43:45.02 +33:35:07.3 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:45.02 +33:35:07.3: 13.23 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:43:45.02 +33:35:07.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.28 14:07:25.16 +39:37:06.8
76.12610 69.88433 galactic Boo Second-epoch detections are separated by 1.1" and 6.7 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 | 14:07:25.16 +39:37:06.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.382+/-0.026 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:25.16 +39:37:06.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:25.16 +39:37:06.8: 13.23 +/- 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,2461258.7083,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.09 13:59:09.83 +40:25:15.3
80.78526 70.70661 galactic CVn Second-epoch detections are separated by 3.3" and 6.8 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 | 13:59:09.83 +40:25:15.3 (user input) | T | P | (position from user input) J-Ks=0.533+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:59:09.83 +40:25:15.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:59:09.83 +40:25:15.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 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,2461258.7083,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.03 13:58:06.67 +41:25:35.0
83.47886 70.21745 galactic CVn Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:06.67 +41:25:35.0 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:06.67 +41:25:35.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:06.67 +41:25:35.0: 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,2461258.7083,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.16 14:02:50.09 +41:25:23.0
81.82128 69.53993 galactic CVn Second-epoch detections are separated by 1.0" and 6.7 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 | 14:02:50.09 +41:25:23.0 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:50.09 +41:25:23.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:50.09 +41:25:23.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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,2461258.7083,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.05 14:03:06.42 +41:03:40.0
80.91365 69.72386 galactic CVn Second-epoch detections are separated by 1.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:03:06.42 +41:03:40.0 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.027 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:06.42 +41:03:40.0: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:06.42 +41:03:40.0: 13.16 +/- 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,2461258.7083,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.15 13:53:40.35 +37:16:51.9
74.54496 73.41398 galactic CVn Second-epoch detections are separated by 1.6" and 6.7 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 | 13:53:40.35 +37:16:51.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.519+/-0.027 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:40.35 +37:16:51.9: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:40.35 +37:16:51.9: 13.06 +/- 0.02 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,2461258.7083,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.17 14:03:02.79 +41:35:31.6
82.12599 69.40306 galactic CVn Second-epoch detections are separated by 2.6" and 6.7 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 | 14:03:02.79 +41:35:31.6 (user input) | T | P | (position from user input) J-Ks=0.250+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:02.79 +41:35:31.6: 13.13 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:02.79 +41:35:31.6: 13.12 +/- 0.02 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,2461258.7083,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.15 13:54:48.60 +37:07:11.5
73.64350 73.31062 galactic CVn Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:54:48.60 +37:07:11.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.329+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:54:48.60 +37:07:11.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:54:48.60 +37:07:11.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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,2461258.7083,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.96 13:56:25.84 +41:51:58.1
85.06306 70.15720 galactic CVn Second-epoch detections are separated by 4.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:56:25.84 +41:51:58.1 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:25.84 +41:51:58.1: 13.09 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:25.84 +41:51:58.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461258.7083,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.04 14:03:15.67 +40:33:06.9
79.68432 70.00862 galactic CVn Second-epoch detections are separated by 1.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:03:15.67 +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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:15.67 +40:33:06.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:15.67 +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-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 12.12 14:05:43.06 +40:34:05.2
78.92609 69.62196 galactic CVn Second-epoch detections are separated by 0.6" and 6.7 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 | 14:05:43.06 +40:34:05.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.300+/-0.027 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:05:43.06 +40:34:05.2: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:05:43.06 +40:34:05.2: 13.00 +/- 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
target,2461258.7083,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.10 14:00:43.23 +40:21:30.5
80.08870 70.51097 galactic CVn Second-epoch detections are separated by 1.6" and 6.7 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 | 14:00:43.23 +40:21:30.5 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:43.23 +40:21:30.5: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:43.23 +40:21:30.5: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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,2461258.7083,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2084 2461258.7083 11.98 13:54:00.04 +41:17:52.2
84.74081 70.87686 galactic CVn Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:54:00.04 +41:17:52.2 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:54:00.04 +41:17:52.2: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:54:00.04 +41:17:52.2: 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,2461258.7083,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 11.98 14:10:08.00 +39:27:16.8
74.92883 69.52622 galactic Boo Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX 4" Gaia DR3 1485540612577549568
Type: ROT
# Max. Min./Amp. JD0 Period
12.580 G 12.600 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:08.00 +39:27:16.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:08.00 +39:27:16.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 1485540612577549568,2461258.7083,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1485540612577549568 20260806.2084 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 06.2084 2461258.7083 12.07 14:43:19.14 +34:27:46.4
56.85893 64.97244 galactic Boo Second-epoch detections are separated by 2.0" and 6.8 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 | 14:43:19.14 +34:27:46.4 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:19.14 +34:27:46.4: 12.99 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:43:19.14 +34:27:46.4: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 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,2461258.7083,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.01 13:58:57.53 +40:43:52.4
81.58839 70.54285 galactic CVn Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:57.53 +40:43:52.4 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:57.53 +40:43:52.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:57.53 +40:43:52.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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,2461258.7083,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.96 14:02:36.57 +40:02:13.6
78.67415 70.41299 galactic CVn Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:02:36.57 +40:02:13.6 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:36.57 +40:02:13.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:36.57 +40:02:13.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461258.7083,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 11.88 14:01:25.98 +40:30:47.0
80.20916 70.30936 galactic CVn Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:01:25.98 +40:30:47.0 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:25.98 +40:30:47.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:25.98 +40:30:47.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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,2461258.7083,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.92 14:03:36.49 +40:44:31.1
80.01322 69.84216 galactic CVn Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J210.9021+40.7419 | 14:03:36.49 +40:44:31.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.270+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:36.49 +40:44:31.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:36.49 +40:44:31.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 J210.9021+40.7419,2461258.7083,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J210.9021+40.7419 20260806.2084 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.87 14:10:19.85 +39:36:23.6
75.24310 69.41498 galactic Boo Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:10:19.85 +39:36:23.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.666+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:19.85 +39:36:23.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:19.85 +39:36:23.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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,2461258.7083,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.94 13:56:43.98 +41:40:42.3
84.54223 70.24259 galactic CVn Second-epoch detections are separated by 1.4" and 6.7 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 | 13:56:43.98 +41:40:42.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.373+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:43.98 +41:40:42.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:43.98 +41:40:42.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461258.7083,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.83 14:00:24.84 +41:06:56.1
81.95747 70.08697 galactic CVn Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:24.84 +41:06:56.1 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.84 +41:06:56.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.84 +41:06:56.1: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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,2461258.7083,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2084 2461258.7083 11.81 14:00:18.19 +41:12:44.9
82.21598 70.04165 galactic CVn Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:18.19 +41:12:44.9 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.027 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:18.19 +41:12:44.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:18.19 +41:12:44.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 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,2461258.7083,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.74 14:00:24.21 +40:22:01.1
80.21925 70.55370 galactic CVn Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:24.21 +40:22:01.1 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.21 +40:22:01.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.21 +40:22:01.1: 12.69 +/- 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,2461258.7083,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.64 14:00:46.27 +41:05:22.7
81.77390 70.05113 galactic CVn Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:00:46.27 +41:05:22.7 (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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:46.27 +41:05:22.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:46.27 +41:05:22.7: 12.62 +/- 0.02 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,2461258.7083,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 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 06.2084 2461258.7083 11.69 13:58:47.56 +40:41:24.9
81.55255 70.59313 galactic CVn Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:47.56 +40:41:24.9 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:47.56 +40:41:24.9: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:47.56 +40:41:24.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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,2461258.7083,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.63 14:02:53.78 +40:55:50.5
80.68552 69.83509 galactic CVn Second-epoch detections are separated by 1.4" and 6.8 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 1497949803887337088 | 14:02:53.54 +40:56:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.368+/-0.026 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:53.78 +40:55:50.5: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:53.78 +40:55:50.5: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 1497949803887337088,2461258.7083,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1497949803887337088 20260806.2084 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.59 14:00:45.52 +41:00:41.2
81.59971 70.10208 galactic CVn Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:45.52 +41:00:41.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:45.52 +41:00:41.2: 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 1498619612627238400,2461258.7083,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.62 14:02:23.90 +40:59:14.9
80.98312 69.87456 galactic CVn Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J210.5994+40.9876 | 14:02:23.90 +40:59:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.338+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:23.90 +40:59:14.9: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:23.90 +40:59:14.9: 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+40.9876,2461258.7083,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.66 13:58:19.77 +40:30:05.0
81.27628 70.78035 galactic CVn Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1498579961489134336 | 13:58:19.73 +40:30:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.596+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:19.77 +40:30:05.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:19.77 +40:30:05.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 1498579961489134336,2461258.7083,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1498579961489134336 20260806.2084 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.46 14:02:09.54 +40:33:39.0
80.07437 70.17068 galactic CVn Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:09.54 +40:33:39.0: 12.52 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:09.54 +40:33:39.0: 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 1497798140002814208,2461258.7083,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.47 14:01:09.73 +41:11:11.0
81.85821 69.93303 galactic CVn Second-epoch detections are separated by 0.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1498716850687059840 | 14:01:09.80 +41:11:11.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.478+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:09.73 +41:11:11.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:09.73 +41:11:11.0: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 1498716850687059840,2461258.7083,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1498716850687059840 20260806.2084 11.47CV 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
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.46 14:06:19.93 +40:29:30.6
78.55401 69.57073 galactic CVn Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1497700936302469632 | 14:06:19.98 +40:29:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.668+/-0.024 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:19.93 +40:29:30.6: 12.39 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:19.93 +40:29:30.6: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 1497700936302469632,2461258.7083,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1497700936302469632 20260806.2084 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 11.38 14:01:11.60 +41:19:05.7
82.14488 69.84524 galactic CVn Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1498720905136167040 | 14:01:11.56 +41:19:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.200+/-0.026 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:11.60 +41:19:05.7: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:11.60 +41:19:05.7: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 1498720905136167040,2461258.7083,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1498720905136167040 20260806.2084 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2084 2461258.7083 12.29 14:02:07.71 +40:51:05.1
80.76149 69.99837 galactic CVn Second-epoch detections are separated by 1.7" and 6.8 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 | 14:02:07.71 +40:51:05.1 (user input) | T | P | (position from user input) J-Ks=0.839+/-0.028 (M)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:07.71 +40:51:05.1: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:07.71 +40:51:05.1: 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,2461258.7083,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260806.2084 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Last image: 2461258.70864630 06.08.2026 05:00:17.040 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 4 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): 5486
Objects passed selection criteria: 5472
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: 3490
Average stars matched: 3397.75 (97.3567 %)
Memory usage VmPeak: 232084 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 00:17:15 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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Last image: 2461258.70864630 06.08.2026 05:00:17.040 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 62
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
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: 13 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): 26967
Objects passed selection criteria: 26891
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 18182.5
Average stars matched: 17513 (96.3179 %)
Memory usage VmPeak: 251424 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 00:18:12 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/TTUQ1b1x1/TTUQ1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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: 2461258.70805391
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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
Saving wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits to local_wcs_cache/
'wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits'
wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits'
wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (1st reference image)
verification OK: wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 14:10:59.063 +37:59:50.07 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 14:10:59.063 +37:59:50.07
Angular distance between the image centers 0.0221 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 14:10:59.302 +38:00:29.58 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 14:10:59.302 +38:00:29.58
Angular distance between the image centers 0.0130 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 14:10:59.063 +37:59:50.07
Second-epoch second image center 14:10:59.302 +38:00:29.58
Angular distance between the image centers 0.01100 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.oz7NYY5CdR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits &> /tmp/tmp.FzGDFDGKhC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits &> /tmp/tmp.g2NgvK3X4s
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits &> /tmp/tmp.dE1RjQIlOt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
The reference image (wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits) and catalog (wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat) found
'wcs_Boo-04-Q1b1x1_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 22.595150
a=0.000000 b=1.000000 c=22.595150
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=6.4)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits (aperture=6.5)
____ 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.4 pix Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
2.9 pix fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
2.8 pix fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Limiting magnitude estimates:
15.3 mag. Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
15.3 mag. Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
12.4 mag. fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
12.1 mag. fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oz7NYY5CdR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=0, passed=5741
Got 5741 stars (including 5440 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_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 4865 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 4861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 5741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 4865 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 5741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 5741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4861 stars left (next iteration limit 5347)
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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=4861 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.378 n_q1=1255 n_q2=1173 n_q3=1225 n_q4=1208 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q1b1x1_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-Q1b1x1_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.FzGDFDGKhC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=0, passed=5807
Got 5807 stars (including 5472 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_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 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 5807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 5807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 5807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4865 stars left (next iteration limit 5351)
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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits N_match=4865 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.377 n_q1=1210 n_q2=1212 n_q3=1189 n_q4=1254 worst_quadrant_to_overall_ratio=1.069
The image catalog is written to wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -region wcs_Boo-04-Q1b1x1_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-Q1b1x1_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.g2NgvK3X4s (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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=38, bad_region=0, passed=1243
Got 1243 stars (including 1204 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 1243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 1162 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1161 matched stars entering correct_measured_positions(), 1157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1161 matched stars entering correct_measured_positions(), 1239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 1162 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1161 matched stars entering correct_measured_positions(), 1241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 1161 matched stars entering correct_measured_positions(), 1241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 1161 stars left (next iteration limit 1277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1161 robust_rms=9.690 arcsec worst_quadrant_rms=10.198 arcsec
SIP_REFIT: SIP order 3 trial: matched=1161 robust_rms=0.380 arcsec worst_quadrant_rms=0.390 arcsec
SIP_REFIT: SIP order 5 trial: matched=1161 robust_rms=0.309 arcsec worst_quadrant_rms=0.345 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1161 robust_rms_before=0.787 arcsec robust_rms_before_corrected=0.313 arcsec robust_rms_after=0.309 arcsec worst_quadrant_rms_before=0.369 worst_quadrant_rms_after=0.345
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.369 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits N_match=1161 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.288 n_q1=250 n_q2=258 n_q3=352 n_q4=301 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits -region wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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.dE1RjQIlOt (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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=0, passed=1265
Got 1265 stars (including 1223 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 1265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 1183 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1182 matched stars entering correct_measured_positions(), 1176 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1182 matched stars entering correct_measured_positions(), 1258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 1183 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1182 matched stars entering correct_measured_positions(), 1258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 1182 matched stars entering correct_measured_positions(), 1258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 1182 stars left (next iteration limit 1300)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1182 robust_rms=9.421 arcsec worst_quadrant_rms=12.462 arcsec
SIP_REFIT: SIP order 3 trial: matched=1182 robust_rms=0.371 arcsec worst_quadrant_rms=0.381 arcsec
SIP_REFIT: SIP order 5 trial: matched=1182 robust_rms=0.300 arcsec worst_quadrant_rms=0.343 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1182 robust_rms_before=0.809 arcsec robust_rms_before_corrected=0.325 arcsec robust_rms_after=0.300 arcsec worst_quadrant_rms_before=0.355 worst_quadrant_rms_after=0.343
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.355 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits N_match=1182 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.291 n_q1=264 n_q2=251 n_q3=363 n_q4=304 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits -region wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits sigma_overall=0.357 worst_q_ratio=1.106
ref2=Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits sigma_overall=0.353 worst_q_ratio=1.069
new1=fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits sigma_overall=0.313 worst_q_ratio=1.146
new2=fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits sigma_overall=0.308 worst_q_ratio=1.094
reference average sigma_overall=0.355 worst_q_ratio=1.0875
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621_astrometric_residuals.png (4861 matched stars from wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181_astrometric_residuals.png (4865 matched stars from wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130_astrometric_residuals.png (1161 matched stars from wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131_astrometric_residuals.png (1182 matched stars from wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits'
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits'
Preparing the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Boo-04-Q1b1x1 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Creating symlink local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits exists and is non-empty
wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (1st reference image)
verification OK: wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 14:10:59.063 +37:59:50.07 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 14:10:59.063 +37:59:50.07
Angular distance between the image centers 0.0221 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 14:10:59.302 +38:00:29.58 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 14:10:59.302 +38:00:29.58
Angular distance between the image centers 0.0130 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 14:10:59.063 +37:59:50.07
Second-epoch second image center 14:10:59.302 +38:00:29.58
Angular distance between the image centers 0.01100 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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.eB0qaFoA6z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits &> /tmp/tmp.Rrl7pniCDq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits &> /tmp/tmp.AKM5czDE17
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits &> /tmp/tmp.JqI1Q7YIHY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits and wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
The reference image (wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits) and catalog (wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat) found
'wcs_Boo-04-Q1b1x1_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 22.496600
a=0.000000 b=1.000000 c=22.496600
From vast_summary.log: estimated ref. image limiting mag.: -7.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=5.1)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 58 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.2 pix Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
2.8 pix fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
2.7 pix fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Limiting magnitude estimates:
15.4 mag. Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
15.4 mag. Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
12.6 mag. fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
12.7 mag. fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eB0qaFoA6z (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=14, blended=1045, bad_region=0, passed=29330
Got 29330 stars (including 28250 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
util/solve_plate_with_UCAC5 got 29330 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 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 29330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 29330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 29330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=4864 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.354 sigma_q4_arcsec=0.372 n_q1=1273 n_q2=1183 n_q3=1188 n_q4=1220 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q1b1x1_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-Q1b1x1_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.Rrl7pniCDq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits' -> 'wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=21, blended=1142, bad_region=1, passed=29296
Got 29296 stars (including 28125 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 29296 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 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 29296 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 43.2)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 29296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 29296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4865 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-04-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits N_match=4865 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.373 n_q1=1227 n_q2=1225 n_q3=1159 n_q4=1254 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Boo-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits -region wcs_Boo-04-Q1b1x1_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-Q1b1x1_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.AKM5czDE17 (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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=98, bad_region=8, passed=7248
Got 7248 stars (including 7132 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 7248 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 4808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 7248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4812 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 7248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 7248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 4806 stars left (next iteration limit 5287)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits N_match=4806 sigma_overall_arcsec=0.598 sigma_q1_arcsec=0.610 sigma_q2_arcsec=0.670 sigma_q3_arcsec=0.552 sigma_q4_arcsec=0.586 n_q1=1079 n_q2=1107 n_q3=1425 n_q4=1195 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits -region wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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.JqI1Q7YIHY (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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=98, bad_region=15, passed=7380
Got 7380 stars (including 7263 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 7380 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 609 to 669 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 7380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 609 to 669 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4802 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 7380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 7380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 4797 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits N_match=4797 sigma_overall_arcsec=0.600 sigma_q1_arcsec=0.630 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.560 sigma_q4_arcsec=0.618 n_q1=1104 n_q2=1067 n_q3=1428 n_q4=1198 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-04-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits -region wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/wcs_fd_Boo-04-Q1b1x1_2026-08-05_23-59-25_20.00sec_-0.00C_LIGHTs_0130.fits
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.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-Q1b1x1_001238_TTUQ1b1x1_3105875_EFTniltM/wcs_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131.fits
Preparing the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:08.41 +39:24:19.1: 11.47 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:31:34.26 +42:51:02.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:49.23 +42:18:23.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:59:51.83 +41:25:51.9: 13.52 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:43.22 +41:28:46.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:57:54.07 +42:10:37.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:11.27 +40:58:45.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:57:27.32 +41:51:47.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:50.53 +40:42:53.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:16.59 +39:21:29.9: 13.50 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:31:34.26 +42:51:02.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 13:31:34.26 +42:51:02.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:49.23 +42:18:23.7: 12.63 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:43.22 +41:28:46.4: 13.30 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:57:54.07 +42:10:37.3: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:11.27 +40:58:45.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:57:27.32 +41:51:47.1: 12.33 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:16.59 +39:21:29.9: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:50.53 +40:42:53.0: 12.71 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:42:08.41 +39:24:19.1: 11.51 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:59:51.83 +41:25:51.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:49.23 +42:18:23.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7027 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 14:06:43.22 +41:28:46.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2675 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Forced photometry filter KEPT candidate at 13:57:54.07 +42:10:37.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9879 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 14:02:11.27 +40:58:45.7: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7244 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 13:57:27.32 +41:51:47.1: ref_mag=12.35 +/- 0.01 new_mean_mag=11.4371 delta=0.91 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:42:08.41 +39:24:19.1: ref_mag=11.49 +/- 0.00 new_mean_mag=11.6673 delta=-0.18 (need > 0.90)
Forced photometry filter KEPT candidate at 14:10:16.59 +39:21:29.9: ref_mag=13.46 +/- 0.02 new_mean_mag=12.4030 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 13:59:51.83 +41:25:51.9: ref_mag=13.50 +/- 0.02 new_mean_mag=12.2984 delta=1.20 (need > 0.90)
Forced photometry filter KEPT candidate at 14:00:50.53 +40:42:53.0: ref_mag=12.72 +/- 0.01 new_mean_mag=11.6712 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:08:32.46 +40:00:56.6: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:08:32.46 +40:00:56.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 14:08:32.46 +40:00:56.6: ref_mag=13.43 +/- 0.02 new_mean_mag=12.2523 delta=1.18 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:54.47 +40:35:06.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:54.47 +40:35:06.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 14:00:54.47 +40:35:06.8: ref_mag=13.43 +/- 0.02 new_mean_mag=12.2341 delta=1.20 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:06.28 +34:11:34.1: 13.46 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:46:06.28 +34:11:34.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter KEPT candidate at 14:46:06.28 +34:11:34.1: ref_mag=13.52 +/- 0.04 new_mean_mag=12.3921 delta=1.13 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:30.81 +40:19:51.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:12:44.99 +37:28:35.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:30.81 +40:19:51.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 14:07:30.81 +40:19:51.4: ref_mag=13.39 +/- 0.02 new_mean_mag=12.2245 delta=1.16 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:10.17 +41:49:26.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:12:44.99 +37:28:35.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 14:12:44.99 +37:28:35.1: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3767 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:10.17 +41:49:26.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:40.74 +41:35:23.9: 13.28 +/- 0.03 detection
Forced photometry filter KEPT candidate at 14:00:10.17 +41:49:26.7: ref_mag=13.28 +/- 0.02 new_mean_mag=12.1503 delta=1.13 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:40.74 +41:35:23.9: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 13:58:40.74 +41:35:23.9: ref_mag=13.26 +/- 0.02 new_mean_mag=12.0836 delta=1.18 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:31.58 +34:15:38.0: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:45.02 +33:35:07.3: 13.23 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:37:31.58 +34:15:38.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 14:37:31.58 +34:15:38.0: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2875 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:07:25.16 +39:37:06.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:59:09.83 +40:25:15.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:43:45.02 +33:35:07.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 14:43:45.02 +33:35:07.3: ref_mag=13.20 +/- 0.02 new_mean_mag=12.0943 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:07:25.16 +39:37:06.8: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 14:07:25.16 +39:37:06.8: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2824 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:59:09.83 +40:25:15.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 13:59:09.83 +40:25:15.3: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0500 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:06.67 +41:25:35.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:50.09 +41:25:23.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:06.67 +41:25:35.0: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 13:58:06.67 +41:25:35.0: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0166 delta=1.12 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:50.09 +41:25:23.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 14:02:50.09 +41:25:23.0: ref_mag=13.20 +/- 0.02 new_mean_mag=12.1135 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:06.42 +41:03:40.0: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:06.42 +41:03:40.0: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 14:03:06.42 +41:03:40.0: ref_mag=13.17 +/- 0.02 new_mean_mag=12.0555 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:53:40.35 +37:16:51.9: 13.18 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:02.79 +41:35:31.6: 13.13 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:53:40.35 +37:16:51.9: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 13:53:40.35 +37:16:51.9: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1416 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:02.79 +41:35:31.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 14:03:02.79 +41:35:31.6: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1571 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:54:48.60 +37:07:11.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:54:48.60 +37:07:11.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 13:54:48.60 +37:07:11.5: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1440 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:25.84 +41:51:58.1: 13.09 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:15.67 +40:33:06.9: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:05:43.06 +40:34:05.2: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:54:00.04 +41:17:52.2: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:43.23 +40:21:30.5: 13.08 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:25.84 +41:51:58.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 13:56:25.84 +41:51:58.1: ref_mag=13.10 +/- 0.02 new_mean_mag=11.9674 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:15.67 +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 14:03:15.67 +40:33:06.9: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0335 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:05:43.06 +40:34:05.2: 13.00 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:43.23 +40:21:30.5: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 14:05:43.06 +40:34:05.2: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0984 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 14:00:43.23 +40:21:30.5: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0825 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:54:00.04 +41:17:52.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 13:54:00.04 +41:17:52.2: ref_mag=13.05 +/- 0.02 new_mean_mag=11.9322 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:08.00 +39:27:16.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:08.00 +39:27:16.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 14:10:08.00 +39:27:16.8: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9746 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:19.14 +34:27:46.4: 12.99 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:43:19.14 +34:27:46.4: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 14:43:19.14 +34:27:46.4: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0410 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:57.53 +40:43:52.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:57.53 +40:43:52.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 13:58:57.53 +40:43:52.4: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0091 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:36.57 +40:02:13.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:25.98 +40:30:47.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:36.57 +40:02:13.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 14:02:36.57 +40:02:13.6: ref_mag=12.94 +/- 0.01 new_mean_mag=11.9702 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:25.98 +40:30:47.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 14:01:25.98 +40:30:47.0: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8836 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:03:36.49 +40:44:31.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:03:36.49 +40:44:31.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 14:03:36.49 +40:44:31.1: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9217 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:10:19.85 +39:36:23.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:56:43.98 +41:40:42.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:10:19.85 +39:36:23.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 14:10:19.85 +39:36:23.6: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8675 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:56:43.98 +41:40:42.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.84 +41:06:56.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:18.19 +41:12:44.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 13:56:43.98 +41:40:42.3: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8651 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.84 +41:06:56.1: 12.74 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:18.19 +41:12:44.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:24.84 +41:06:56.1: ref_mag=12.74 +/- 0.01 new_mean_mag=11.8151 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 14:00:18.19 +41:12:44.9: ref_mag=12.72 +/- 0.01 new_mean_mag=11.8095 delta=0.91 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:24.21 +40:22:01.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:24.21 +40:22:01.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:24.21 +40:22:01.1: ref_mag=12.70 +/- 0.01 new_mean_mag=11.6737 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:46.27 +41:05:22.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:46.27 +41:05:22.7: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:46.27 +41:05:22.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6348 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:47.56 +40:41:24.9: 12.69 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:47.56 +40:41:24.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 13:58:47.56 +40:41:24.9: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6906 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:53.78 +40:55:50.5: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:00:45.52 +41:00:41.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:23.90 +40:59:14.9: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:53.78 +40:55:50.5: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 14:02:53.78 +40:55:50.5: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6305 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:00:45.52 +41:00:41.2: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 14:00:45.52 +41:00:41.2: ref_mag=12.59 +/- 0.01 new_mean_mag=11.5694 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:23.90 +40:59:14.9: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 14:02:23.90 +40:59:14.9: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6098 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 13:58:19.77 +40:30:05.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:09.54 +40:33:39.0: 12.52 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 13:58:19.77 +40:30:05.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 13:58:19.77 +40:30:05.0: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5947 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:09.54 +40:33:39.0: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 14:02:09.54 +40:33:39.0: ref_mag=12.52 +/- 0.01 new_mean_mag=11.4573 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:09.73 +41:11:11.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:09.73 +41:11:11.0: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 14:01:09.73 +41:11:11.0: ref_mag=12.45 +/- 0.01 new_mean_mag=11.4720 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:06:19.93 +40:29:30.6: 12.39 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:06:19.93 +40:29:30.6: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 14:06:19.93 +40:29:30.6: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4347 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:01:11.60 +41:19:05.7: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:01:11.60 +41:19:05.7: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 14:01:11.60 +41:19:05.7: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3654 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:02:07.71 +40:51:05.1: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-06-08_01-12-41_20.00sec_5.00C_LIGHT_0181.fits at 14:02:07.71 +40:51:05.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 14:02:07.71 +40:51:05.1: ref_mag=13.65 +/- 0.03 new_mean_mag=12.2586 delta=1.39 (need > 0.90)
Adding exclusion_list_local.txt__out02474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05840.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__out06360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06991.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__out07433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26266.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 79s
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: 28s
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Considering the candidate 32422_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 32422_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 32438_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 32438_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
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Considering the candidate 03644_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 03644_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 02474_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 02474_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 06237_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06237_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 06948_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06948_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 02776_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 02776_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04841_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04841_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 10866_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 10866_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04898_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04898_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 09050_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 09050_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 07350_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07350_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 23772_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 23772_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 08140_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 08140_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 16468_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 16468_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 03819_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 03819_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04429_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04429_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 15766_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 15766_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 13:50:44.21 +37:37:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23596_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 23596_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 26266_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 26266_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 10160_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 10160_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 07788_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07788_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04876_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04876_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04956_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04956_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 06043_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06043_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 16812_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 16812_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 04480_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04480_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 17354_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 17354_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 03618_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 03618_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 07455_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07455_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 07433_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07433_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 07982_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07982_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 05178_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05178_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
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Considering the candidate 19397_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 19397_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 13:35:03.82 +33:03:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10591_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 10591_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24418_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 24418_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06896_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06896_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08934_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 08934_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07540_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07540_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06923_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06923_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10202_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 10202_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04148_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 04148_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05840_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05840_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05574_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05574_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07934_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07934_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05896_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05896_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06991_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06991_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06360_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06360_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06125_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06125_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06216_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06216_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07514_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07514_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07400_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07400_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05649_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05649_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07641_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 07641_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05250_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 05250_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21466_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 21466_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 13:48:44.70 +33:43:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09655_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
The candidate 09655_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131 did not pass the final checks
**** FOUND 13:48:57.21 +39:32:32.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06587_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
Preparing report for the candidate 06587_fd_Boo-04-Q1b1x1_2026-08-06_00-00-17_20.00sec_-0.00C_LIGHTs_0131
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 112s
Prepared the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:00:49.23 +42:18:23.7
13:57:54.07 +42:10:37.3
13:56:25.84 +41:51:58.1
13:57:27.32 +41:51:47.1
14:00:10.17 +41:49:26.7
13:56:43.98 +41:40:42.3
13:58:40.74 +41:35:23.9
14:03:02.79 +41:35:31.6
14:06:43.22 +41:28:46.4
13:58:06.67 +41:25:35.0
13:59:51.83 +41:25:51.9
14:02:50.09 +41:25:23.0
13:54:00.04 +41:17:52.2
14:01:11.60 +41:19:05.7
14:00:18.19 +41:12:44.9
14:01:09.73 +41:11:11.0
14:00:24.84 +41:06:56.1
14:00:46.27 +41:05:22.7
14:03:06.42 +41:03:40.0
14:00:45.52 +41:00:41.2
14:02:23.90 +40:59:14.9
14:02:11.27 +40:58:45.7
14:02:53.78 +40:55:50.5
14:02:07.71 +40:51:05.1
13:58:57.53 +40:43:52.4
14:03:36.49 +40:44:31.1
14:00:50.53 +40:42:53.0
13:58:47.56 +40:41:24.9
14:00:54.47 +40:35:06.8
14:02:09.54 +40:33:39.0
14:05:43.06 +40:34:05.2
14:03:15.67 +40:33:06.9
13:58:19.77 +40:30:05.0
14:01:25.98 +40:30:47.0
14:06:19.93 +40:29:30.6
13:59:09.83 +40:25:15.3
14:00:24.21 +40:22:01.1
14:00:43.23 +40:21:30.5
14:07:30.81 +40:19:51.4
14:02:36.57 +40:02:13.6
14:08:32.46 +40:00:56.6
14:07:25.16 +39:37:06.8
14:10:19.85 +39:36:23.6
14:10:08.00 +39:27:16.8
14:10:16.59 +39:21:29.9
14:12:44.99 +37:28:35.1
13:53:40.35 +37:16:51.9
13:54:48.60 +37:07:11.5
14:37:31.58 +34:15:38.0
14:46:06.28 +34:11:34.1
14:43:19.14 +34:27:46.4
14:43:45.02 +33:35:07.3
########### Completed Boo-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
13:57:27.32 +41:51:47.1
14:00:49.23 +42:18:23.7
14:02:11.27 +40:58:45.7
14:00:50.53 +40:42:53.0
13:57:54.07 +42:10:37.3
14:06:43.22 +41:28:46.4
14:10:16.59 +39:21:29.9
13:59:51.83 +41:25:51.9
14:08:32.46 +40:00:56.6
14:00:54.47 +40:35:06.8
14:46:06.28 +34:11:34.1
14:07:30.81 +40:19:51.4
14:12:44.99 +37:28:35.1
14:00:10.17 +41:49:26.7
13:58:40.74 +41:35:23.9
14:37:31.58 +34:15:38.0
14:43:45.02 +33:35:07.3
14:07:25.16 +39:37:06.8
13:59:09.83 +40:25:15.3
13:58:06.67 +41:25:35.0
14:02:50.09 +41:25:23.0
14:03:06.42 +41:03:40.0
13:53:40.35 +37:16:51.9
14:03:02.79 +41:35:31.6
13:54:48.60 +37:07:11.5
13:56:25.84 +41:51:58.1
14:03:15.67 +40:33:06.9
14:05:43.06 +40:34:05.2
14:00:43.23 +40:21:30.5
13:54:00.04 +41:17:52.2
14:10:08.00 +39:27:16.8
14:43:19.14 +34:27:46.4
13:58:57.53 +40:43:52.4
14:02:36.57 +40:02:13.6
14:01:25.98 +40:30:47.0
14:03:36.49 +40:44:31.1
14:10:19.85 +39:36:23.6
13:56:43.98 +41:40:42.3
14:00:24.84 +41:06:56.1
14:00:18.19 +41:12:44.9
14:00:24.21 +40:22:01.1
14:00:46.27 +41:05:22.7
13:58:47.56 +40:41:24.9
14:02:53.78 +40:55:50.5
14:00:45.52 +41:00:41.2
14:02:23.90 +40:59:14.9
13:58:19.77 +40:30:05.0
14:02:09.54 +40:33:39.0
14:01:09.73 +41:11:11.0
14:06:19.93 +40:29:30.6
14:01:11.60 +41:19:05.7
14:02:07.71 +40:51:05.1
###################################################################################
13:57:27.32 +41:51:47.1 -- not an asteroid (will add it to exclusion list)
14:00:49.23 +42:18:23.7 -- not an asteroid (will add it to exclusion list)
14:02:11.27 +40:58:45.7 -- not an asteroid (will add it to exclusion list)
14:00:50.53 +40:42:53.0 -- not an asteroid (will add it to exclusion list)
13:57:54.07 +42:10:37.3 -- not an asteroid (will add it to exclusion list)
14:06:43.22 +41:28:46.4 -- not an asteroid (will add it to exclusion list)
14:10:16.59 +39:21:29.9 -- not an asteroid (will add it to exclusion list)
13:59:51.83 +41:25:51.9 -- not an asteroid (will add it to exclusion list)
14:08:32.46 +40:00:56.6 -- not an asteroid (will add it to exclusion list)
14:00:54.47 +40:35:06.8 -- not an asteroid (will add it to exclusion list)
14:46:06.28 +34:11:34.1 -- not an asteroid (will add it to exclusion list)
14:07:30.81 +40:19:51.4 -- not an asteroid (will add it to exclusion list)
14:12:44.99 +37:28:35.1 -- not an asteroid (will add it to exclusion list)
14:00:10.17 +41:49:26.7 -- not an asteroid (will add it to exclusion list)
13:58:40.74 +41:35:23.9 -- not an asteroid (will add it to exclusion list)
14:37:31.58 +34:15:38.0 -- not an asteroid (will add it to exclusion list)
14:43:45.02 +33:35:07.3 -- not an asteroid (will add it to exclusion list)
14:07:25.16 +39:37:06.8 -- not an asteroid (will add it to exclusion list)
13:59:09.83 +40:25:15.3 -- not an asteroid (will add it to exclusion list)
13:58:06.67 +41:25:35.0 -- not an asteroid (will add it to exclusion list)
14:02:50.09 +41:25:23.0 -- not an asteroid (will add it to exclusion list)
14:03:06.42 +41:03:40.0 -- not an asteroid (will add it to exclusion list)
13:53:40.35 +37:16:51.9 -- not an asteroid (will add it to exclusion list)
14:03:02.79 +41:35:31.6 -- not an asteroid (will add it to exclusion list)
13:54:48.60 +37:07:11.5 -- not an asteroid (will add it to exclusion list)
13:56:25.84 +41:51:58.1 -- not an asteroid (will add it to exclusion list)
14:03:15.67 +40:33:06.9 -- not an asteroid (will add it to exclusion list)
14:05:43.06 +40:34:05.2 -- not an asteroid (will add it to exclusion list)
14:00:43.23 +40:21:30.5 -- not an asteroid (will add it to exclusion list)
13:54:00.04 +41:17:52.2 -- not an asteroid (will add it to exclusion list)
14:10:08.00 +39:27:16.8 -- not an asteroid (will add it to exclusion list)
14:43:19.14 +34:27:46.4 -- not an asteroid (will add it to exclusion list)
13:58:57.53 +40:43:52.4 -- not an asteroid (will add it to exclusion list)
14:02:36.57 +40:02:13.6 -- not an asteroid (will add it to exclusion list)
14:01:25.98 +40:30:47.0 -- not an asteroid (will add it to exclusion list)
14:03:36.49 +40:44:31.1 -- not an asteroid (will add it to exclusion list)
14:10:19.85 +39:36:23.6 -- not an asteroid (will add it to exclusion list)
13:56:43.98 +41:40:42.3 -- not an asteroid (will add it to exclusion list)
14:00:24.84 +41:06:56.1 -- not an asteroid (will add it to exclusion list)
14:00:18.19 +41:12:44.9 -- not an asteroid (will add it to exclusion list)
14:00:24.21 +40:22:01.1 -- not an asteroid (will add it to exclusion list)
14:00:46.27 +41:05:22.7 -- not an asteroid (will add it to exclusion list)
13:58:47.56 +40:41:24.9 -- not an asteroid (will add it to exclusion list)
14:02:53.78 +40:55:50.5 -- not an asteroid (will add it to exclusion list)
14:00:45.52 +41:00:41.2 -- not an asteroid (will add it to exclusion list)
14:02:23.90 +40:59:14.9 -- not an asteroid (will add it to exclusion list)
13:58:19.77 +40:30:05.0 -- not an asteroid (will add it to exclusion list)
14:02:09.54 +40:33:39.0 -- not an asteroid (will add it to exclusion list)
14:01:09.73 +41:11:11.0 -- not an asteroid (will add it to exclusion list)
14:06:19.93 +40:29:30.6 -- not an asteroid (will add it to exclusion list)
14:01:11.60 +41:19:05.7 -- not an asteroid (will add it to exclusion list)
14:02:07.71 +40:51:05.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
13:53:40.35 +37:16:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:54:00.04 +41:17:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:54:48.60 +37:07:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:56:25.84 +41:51:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:56:43.98 +41:40:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:57:27.32 +41:51:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:57:54.07 +42:10:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:06.67 +41:25:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:19.77 +40:30:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:40.74 +41:35:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:47.56 +40:41:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:58:57.53 +40:43:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:59:09.83 +40:25:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:59:51.83 +41:25:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:10.17 +41:49:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:18.19 +41:12:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:24.21 +40:22:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:24.84 +41:06:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:43.23 +40:21:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:45.52 +41:00:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:46.27 +41:05:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:49.23 +42:18:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:50.53 +40:42:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:00:54.47 +40:35:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:09.73 +41:11:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:11.60 +41:19:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:01:25.98 +40:30:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:07.71 +40:51:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:09.54 +40:33:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:11.27 +40:58:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:23.90 +40:59:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:36.57 +40:02:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:50.09 +41:25:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:02:53.78 +40:55:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:02.79 +41:35:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:06.42 +41:03:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:15.67 +40:33:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:03:36.49 +40:44:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:05:43.06 +40:34:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:06:19.93 +40:29:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:06:43.22 +41:28:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:25.16 +39:37:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:30.81 +40:19:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:32.46 +40:00:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:08.00 +39:27:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:16.59 +39:21:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:19.85 +39:36:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:44.99 +37:28:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:37:31.58 +34:15:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:19.14 +34:27:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:45.02 +33:35:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:06.28 +34:11:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
13:53:40.35 +37:16:51.9 -- not a known variable star
13:54:00.04 +41:17:52.2 -- not a known variable star
13:54:48.60 +37:07:11.5 -- not a known variable star
13:56:25.84 +41:51:58.1 -- not a known variable star
13:56:43.98 +41:40:42.3 -- not a known variable star
13:57:27.32 +41:51:47.1 -- a known variable star
13:57:54.07 +42:10:37.3 -- not a known variable star
13:58:06.67 +41:25:35.0 -- not a known variable star
13:58:19.77 +40:30:05.0 -- not a known variable star
13:58:40.74 +41:35:23.9 -- not a known variable star
13:58:47.56 +40:41:24.9 -- not a known variable star
13:58:57.53 +40:43:52.4 -- not a known variable star
13:59:09.83 +40:25:15.3 -- not a known variable star
13:59:51.83 +41:25:51.9 -- not a known variable star
14:00:10.17 +41:49:26.7 -- not a known variable star
14:00:18.19 +41:12:44.9 -- not a known variable star
14:00:24.21 +40:22:01.1 -- not a known variable star
14:00:24.84 +41:06:56.1 -- not a known variable star
14:00:43.23 +40:21:30.5 -- not a known variable star
14:00:45.52 +41:00:41.2 -- not a known variable star
14:00:46.27 +41:05:22.7 -- not a known variable star
14:00:49.23 +42:18:23.7 -- not a known variable star
14:00:50.53 +40:42:53.0 -- not a known variable star
14:00:54.47 +40:35:06.8 -- not a known variable star
14:01:09.73 +41:11:11.0 -- not a known variable star
14:01:11.60 +41:19:05.7 -- not a known variable star
14:01:25.98 +40:30:47.0 -- not a known variable star
14:02:07.71 +40:51:05.1 -- not a known variable star
14:02:09.54 +40:33:39.0 -- not a known variable star
14:02:11.27 +40:58:45.7 -- not a known variable star
14:02:23.90 +40:59:14.9 -- not a known variable star
14:02:36.57 +40:02:13.6 -- not a known variable star
14:02:50.09 +41:25:23.0 -- not a known variable star
14:02:53.78 +40:55:50.5 -- not a known variable star
14:03:02.79 +41:35:31.6 -- not a known variable star
14:03:06.42 +41:03:40.0 -- not a known variable star
14:03:15.67 +40:33:06.9 -- not a known variable star
14:03:36.49 +40:44:31.1 -- not a known variable star
14:05:43.06 +40:34:05.2 -- not a known variable star
14:06:19.93 +40:29:30.6 -- not a known variable star
14:06:43.22 +41:28:46.4 -- not a known variable star
14:07:25.16 +39:37:06.8 -- not a known variable star
14:07:30.81 +40:19:51.4 -- not a known variable star
14:08:32.46 +40:00:56.6 -- not a known variable star
14:10:08.00 +39:27:16.8 -- a known variable star
14:10:16.59 +39:21:29.9 -- not a known variable star
14:10:19.85 +39:36:23.6 -- not a known variable star
14:12:44.99 +37:28:35.1 -- not a known variable star
14:37:31.58 +34:15:38.0 -- not a known variable star
14:43:19.14 +34:27:46.4 -- not a known variable star
14:43:45.02 +33:35:07.3 -- not a known variable star
14:46:06.28 +34:11:34.1 -- not a known variable star
Found 50 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (excluding asteroids and hot pixels, 50 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.70805391 -observatory V36
07:45:33.92 +20:23:14.4 Mercury (-0.3mag)
11:55:38.64 -00:03:40.1 Venus (-4.3mag)
05:43:24.36 +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)
04:11:29.62 +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)
02:46:13.18 +20:31:27.8 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 00:17 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461258.70805391:
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 +18:46:10.0 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 00:17 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.70805391:
18:55:36.97 -24:03:55.2 JWST
17:13:13.33 +42:04:23.6 Chandra
09:20:25.97 -52:45:01.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 00:17 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.70805391 -observatory V36
03:11:22.41 +17:12:22.8 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 +36:43:30.4 16.7mag P/2021 N1 (ZTF)
22:40:17.39 +31:33:58.7 17.3mag C/2022 E2 (ATLAS)
06:41:28.07 +26:34:32.3 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)
21:13:26.18 +66:13:59.9 17.9mag C/2023 H5 (Lemmon)
15:49:55.20 -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 -26:26:58.9 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
11:03:34.59 +05:18:06.2 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
04:00:41.28 +16:05:25.6 17.6mag 112P/Urata-Niijima
05:49:48.94 +30:30:58.1 16.3mag 114P/Wiseman-Skiff
09:13:42.56 +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
06:25:03.39 +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
07:09:10.98 +37:41:19.6 15.8mag 162P/SidingSpring
15:50:12.57 +39:28:48.4 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
20:23:44.74 -52:50:55.5 17.8mag 259P/Garradd
03:16:14.28 +24:18:46.1 15.4mag 260P/McNaught
06:59:17.27 +37:45:17.9 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 00:17 comets.txt
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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 00:17 asassn_transients_list.txt
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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 00:17 tocp_transients_list.txt
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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 00:17 tns_transients_list.txt
