This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6
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 06.2246 2461258.7246 12.74 13:36:50.74 +56:24:10.7
110.49653 59.61552 galactic UMa Second-epoch detections are separated by 2.5" and 0.5 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 | 13:36:50.74 +56:24:10.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:36:50.74 +56:24:10.7: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:36:50.74 +56:24:10.7: 15.96 +/- 99.00 upperlimit
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!
TCP 2026 08 06.2246* 13 36 50.74 +56 24 10.7 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.74,0.05,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 20260806.2246 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 13.01 14:52:19.92 +56:35:58.8
95.15627 53.51425 galactic Dra Second-epoch detections are separated by 7.4" and 0.4 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 | 14:52:19.92 +56:35:58.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:52:19.92 +56:35:58.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:52:19.92 +56:35:58.8: 15.89 +/- 99.00 upperlimit
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,2461258.7246,13.01,0.05,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 20260806.2246 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.46 13:17:05.39 +55:17:50.1
115.28621 61.44857 galactic UMa Second-epoch detections are separated by 6.4" and 0.4 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 | 13:17:05.39 +55:17:50.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:05.39 +55:17:50.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:05.39 +55:17:50.1: 15.94 +/- 99.00 upperlimit
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!
TCP 2026 08 06.2246* 13 17 05.39 +55 17 50.1 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.46,0.05,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
target 20260806.2246 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 13.21 14:25:00.92 +55:32:49.9
98.61589 56.94015 galactic UMa Second-epoch detections are separated by 3.1" and 0.4 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 | 14:25:00.92 +55:32:49.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:25:00.92 +55:32:49.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:25:00.92 +55:32:49.9: 16.00 +/- 99.00 upperlimit
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!
TCP 2026 08 06.2246* 14 25 00.92 +55 32 49.9 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,13.21,0.05,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 20260806.2246 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.96 13:15:28.69 +53:50:13.8
115.13033 62.92543 galactic UMa Second-epoch detections are separated by 0.6" and 0.8 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 | 13:15:28.69 +53:50:13.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.274+/-0.032 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:28.69 +53:50:13.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:28.69 +53:50:13.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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!
TCP 2026 08 06.2246* 13 15 28.69 +53 50 13.8 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,11.96,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.20 13:14:38.48 +54:37:03.8
115.72699 62.18475 galactic UMa Second-epoch detections are separated by 1.8" and 0.6 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 | 13:14:38.48 +54:37:03.8 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.028 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:38.48 +54:37:03.8: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:38.48 +54:37:03.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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!
TCP 2026 08 06.2246* 13 14 38.48 +54 37 03.8 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.20,0.05,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 20260806.2246 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.44 13:23:14.46 +54:05:55.4
112.84814 62.40249 galactic UMa Second-epoch detections are separated by 0.1" and 0.8 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 | 13:23:14.46 +54:05:55.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:23:14.46 +54:05:55.4: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:23:14.46 +54:05:55.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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!
TCP 2026 08 06.2246* 13 23 14.46 +54 05 55.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.44,0.05,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 20260806.2246 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.58 14:51:54.75 +51:47:00.2
88.64200 56.56386 galactic Boo Second-epoch detections are separated by 2.6" and 0.9 pix
The object was found in VSX14" Gaia DR3 1593596767064562304
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.000 G M
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:51:54.75 +51:47:00.2: 13.60 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:51:54.75 +51:47:00.2: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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
Gaia DR3 1593596767064562304,2461258.7246,12.58,0.05,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 1593596767064562304 20260806.2246 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 12.55 14:54:05.90 +54:01:27.5
91.47973 54.95683 galactic Boo Second-epoch detections are separated by 2.4" and 0.6 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 | 14:54:05.90 +54:01:27.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.261+/-0.032 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:54:05.90 +54:01:27.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:54:05.90 +54:01:27.5: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461258.7246,12.55,0.05,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 20260806.2246 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.44 13:19:19.92 +54:45:46.5
114.37921 61.89971 galactic UMa Second-epoch detections are separated by 3.8" and 0.4 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 | 13:19:19.92 +54:45:46.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.397+/-0.026 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:19.92 +54:45:46.5: 13.53 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:19.92 +54:45:46.5: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 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!
TCP 2026 08 06.2246* 13 19 19.92 +54 45 46.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.44,0.05,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 20260806.2246 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.61 14:57:06.97 +54:46:29.1
92.04073 54.15048 galactic Boo Second-epoch detections are separated by 1.2" and 0.9 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 | Large-amplitude variable Gaia DR2 1606358214412143488 | 14:57:06.97 +54:46:29.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.503+/-0.031 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:57:06.97 +54:46:29.1: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:57:06.97 +54:46:29.1: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 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
Large-amplitude variable Gaia DR2 1606358214412143488,2461258.7246,12.61,0.05,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
Large-amplitude variable Gaia DR2 1606358214412143488 20260806.2246 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.41 13:14:35.36 +55:29:52.6
116.09562 61.32195 galactic UMa Second-epoch detections are separated by 2.5" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J198.6541+55.4960 | 13:14:35.36 +55:29:52.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:35.36 +55:29:52.6: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:35.36 +55:29:52.6: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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!
TCP 2026 08 06.2246* 13 14 35.36 +55 29 52.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J198.6541+55.4960,2461258.7246,12.41,0.05,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 J198.6541+55.4960 20260806.2246 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 12.38 13:19:17.33 +54:55:06.5
114.46735 61.74970 galactic UMa Second-epoch detections are separated by 3.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:17.33 +54:55:06.5 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.025 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:17.33 +54:55:06.5: 13.48 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:17.33 +54:55:06.5: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 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!
TCP 2026 08 06.2246* 13 19 17.33 +54 55 06.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.38,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.26 13:21:47.47 +49:08:16.4
110.03700 67.22344 galactic CVn Second-epoch detections are separated by 2.0" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:47.47 +49:08:16.4 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:47.47 +49:08:16.4: 13.49 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:47.47 +49:08:16.4: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461258.7246,12.26,0.05,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 20260806.2246 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.41 13:20:36.73 +55:51:52.5
114.53903 60.78573 galactic UMa Second-epoch detections are separated by 2.1" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:36.73 +55:51:52.5 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.026 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:36.73 +55:51:52.5: 13.44 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:36.73 +55:51:52.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 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!
TCP 2026 08 06.2246* 13 20 36.73 +55 51 52.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.41,0.05,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 20260806.2246 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 12.38 13:19:24.69 +56:40:02.0
115.23259 60.04090 galactic UMa Second-epoch detections are separated by 3.1" and 0.6 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 | 13:19:24.69 +56:40:02.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.413+/-0.030 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:24.69 +56:40:02.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:24.69 +56:40:02.0: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2246* 13 19 24.69 +56 40 02.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.38,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.37 13:21:23.47 +54:20:09.7
113.54219 62.24278 galactic UMa Second-epoch detections are separated by 2.3" and 0.4 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 | 13:21:23.47 +54:20:09.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:23.47 +54:20:09.7: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:23.47 +54:20:09.7: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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!
TCP 2026 08 06.2246* 13 21 23.47 +54 20 09.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.37,0.05,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 20260806.2246 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.40 13:20:38.77 +56:36:11.9
114.87260 60.06557 galactic UMa Second-epoch detections are separated by 1.6" and 0.9 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 | 13:20:38.77 +56:36:11.9 (user input) | T | P | (position from user input) J-Ks=0.809+/-0.029 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:38.77 +56:36:11.9: 13.40 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:38.77 +56:36:11.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2246* 13 20 38.77 +56 36 11.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.40,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.13 13:20:15.37 +49:10:17.9
110.68259 67.26555 galactic CVn Second-epoch detections are separated by 3.4" and 1.4 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 | 13:20:15.37 +49:10:17.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.371+/-0.032 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:15.37 +49:10:17.9: 13.37 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:15.37 +49:10:17.9: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461258.7246,12.13,0.05,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 20260806.2246 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.27 13:21:27.54 +54:41:03.9
113.70625 61.90283 galactic UMa Second-epoch detections are separated by 0.6" and 0.7 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 | 13:21:27.54 +54:41:03.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.385+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:27.54 +54:41:03.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:27.54 +54:41:03.9: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2246* 13 21 27.54 +54 41 03.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.27,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.35 13:29:18.84 +54:46:28.5
111.46046 61.50206 galactic UMa Second-epoch detections are separated by 3.8" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:18.84 +54:46:28.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.378+/-0.040 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:29:18.84 +54:46:28.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:29:18.84 +54:46:28.5: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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!
TCP 2026 08 06.2246* 13 29 18.84 +54 46 28.5 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.35,0.05,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 20260806.2246 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.34 13:17:07.02 +56:17:38.8
115.69939 60.47209 galactic UMa Second-epoch detections are separated by 2.6" and 1.2 pix
The object was found in VSX 1" Gaia DR3 1566153296136118656
Type: ROT
# Max. Min./Amp. JD0 Period
13.000 G 13.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:07.02 +56:17:38.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:07.02 +56:17:38.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 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!
TCP 2026 08 06.2246* 13 17 07.02 +56 17 38.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566153296136118656,2461258.7246,12.34,0.05,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 1566153296136118656 20260806.2246 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.42 13:49:19.07 +53:57:26.8
105.20173 61.13326 galactic UMa Second-epoch detections are separated by 1.5" and 0.9 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 | 13:49:19.07 +53:57:26.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.032 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:49:19.07 +53:57:26.8: 13.33 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:49:19.07 +53:57:26.8: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 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!
TCP 2026 08 06.2246* 13 49 19.07 +53 57 26.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.42,0.05,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 20260806.2246 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.31 13:22:25.92 +52:52:38.0
112.38273 63.61159 galactic UMa Second-epoch detections are separated by 1.7" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:25.92 +52:52:38.0 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.380+/-0.029 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:25.92 +52:52:38.0: 13.29 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:25.92 +52:52:38.0: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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!
TCP 2026 08 06.2246* 13 22 25.92 +52 52 38.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.31,0.05,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 20260806.2246 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.19 13:15:03.48 +53:43:25.6
115.21335 63.04907 galactic UMa Second-epoch detections are separated by 1.8" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:03.48 +53:43:25.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.416+/-0.029 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:03.48 +53:43:25.6: 13.30 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:03.48 +53:43:25.6: 13.31 +/- 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!
TCP 2026 08 06.2246* 13 15 03.48 +53 43 25.6 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.19,0.05,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 20260806.2246 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.30 13:17:05.05 +55:07:28.8
115.21236 61.61753 galactic UMa Second-epoch detections are separated by 3.4" and 0.6 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 | 13:17:05.05 +55:07:28.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:05.05 +55:07:28.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:05.05 +55:07:28.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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!
TCP 2026 08 06.2246* 13 17 05.05 +55 07 28.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.30,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.16 13:17:53.49 +52:06:03.7
113.46040 64.53801 galactic CVn Second-epoch detections are separated by 2.5" and 1.1 pix
The object was found in VSX 1" Gaia DR3 1562843564275182080
Type: ROT
# Max. Min./Amp. JD0 Period
12.950 G 12.980 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:53.49 +52:06:03.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:53.49 +52:06:03.7: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562843564275182080,2461258.7246,12.16,0.05,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
Gaia DR3 1562843564275182080 20260806.2246 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 06.2246 2461258.7246 12.04 13:19:58.55 +49:27:41.4
111.00848 67.00084 galactic CVn Second-epoch detections are separated by 1.1" and 0.9 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 | 13:19:58.55 +49:27:41.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:58.55 +49:27:41.4: 13.26 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:58.55 +49:27:41.4: 13.20 +/- 0.04 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,2461258.7246,12.04,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.13 13:20:24.39 +50:07:43.8
111.31399 66.34090 galactic CVn Second-epoch detections are separated by 0.6" and 0.9 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 | 13:20:24.39 +50:07:43.8 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.031 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:24.39 +50:07:43.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:24.39 +50:07:43.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461258.7246,12.13,0.05,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 20260806.2246 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.99 13:20:17.94 +49:38:30.1
111.01053 66.81318 galactic CVn Second-epoch detections are separated by 1.0" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:17.94 +49:38:30.1 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:17.94 +49:38:30.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:17.94 +49:38:30.1: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 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,2461258.7246,11.99,0.05,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 20260806.2246 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.01 13:19:53.28 +49:24:13.3
111.00169 67.06033 galactic CVn Second-epoch detections are separated by 2.8" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:53.28 +49:24:13.3 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.034 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:53.28 +49:24:13.3: 13.27 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:53.28 +49:24:13.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461258.7246,12.01,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.23 13:16:24.05 +55:27:09.5
115.55266 61.31652 galactic UMa Second-epoch detections are separated by 3.2" and 1.4 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 | 13:16:24.05 +55:27:09.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.593+/-0.030 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:24.05 +55:27:09.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:24.05 +55:27:09.5: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 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!
TCP 2026 08 06.2246* 13 16 24.05 +55 27 09.5 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.23,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.25 13:20:39.24 +50:06:34.2
111.20556 66.34831 galactic CVn Second-epoch detections are separated by 1.0" and 0.7 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 | 13:20:39.24 +50:06:34.2 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:39.24 +50:06:34.2: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:39.24 +50:06:34.2: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461258.7246,12.25,0.05,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 20260806.2246 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.29 13:24:26.24 +55:08:38.4
113.08396 61.34881 galactic UMa Second-epoch detections are separated by 0.6" and 0.9 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 | 13:24:26.24 +55:08:38.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.379+/-0.031 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:26.24 +55:08:38.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:26.24 +55:08:38.4: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 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!
TCP 2026 08 06.2246* 13 24 26.24 +55 08 38.4 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.29,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.17 13:20:12.90 +49:51:22.8
111.19673 66.61111 galactic CVn Second-epoch detections are separated by 0.9" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:12.90 +49:51:22.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:12.90 +49:51:22.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:12.90 +49:51:22.8: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.17,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.03 13:20:46.90 +49:15:28.3
110.53533 67.15810 galactic CVn Second-epoch detections are separated by 2.9" and 1.0 pix
The object was found in VSX 1" Gaia DR3 1553163704422133760
Type: ROT
# Max. Min./Amp. JD0 Period
12.870 G 12.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:46.90 +49:15:28.3: 13.17 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:46.90 +49:15:28.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1553163704422133760,2461258.7246,12.03,0.05,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
Gaia DR3 1553163704422133760 20260806.2246 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 06.2246 2461258.7246 12.16 13:17:23.43 +56:10:13.7
115.57266 60.58541 galactic UMa Second-epoch detections are separated by 0.6" and 0.7 pix
The object was found in VSX 2" Gaia DR3 1566135021052026880
Type: ROT
# Max. Min./Amp. JD0 Period
12.380 G 12.410 G M
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:23.43 +56:10:13.7: 13.21 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:23.43 +56:10:13.7: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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!
TCP 2026 08 06.2246* 13 17 23.43 +56 10 13.7 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566135021052026880,2461258.7246,12.16,0.05,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
Gaia DR3 1566135021052026880 20260806.2246 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 06.2246 2461258.7246 12.07 13:20:10.48 +49:23:34.4
110.87909 67.05744 galactic CVn Second-epoch detections are separated by 4.3" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:10.48 +49:23:34.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:10.48 +49:23:34.4: 13.17 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:10.48 +49:23:34.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.07,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.29 13:18:09.50 +56:50:49.0
115.64403 59.90162 galactic UMa Second-epoch detections are separated by 0.7" and 0.7 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 | 13:18:09.50 +56:50:49.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:18:09.50 +56:50:49.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:18:09.50 +56:50:49.0: 13.27 +/- 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!
TCP 2026 08 06.2246* 13 18 09.50 +56 50 49.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.29,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.15 13:22:37.33 +53:41:48.0
112.80763 62.81433 galactic UMa Second-epoch detections are separated by 1.3" and 0.6 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 | 13:22:37.33 +53:41:48.0 (user input) | T | P | (position from user input) J-Ks=0.578+/-0.032 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:37.33 +53:41:48.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:37.33 +53:41:48.0: 13.09 +/- 0.03 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!
TCP 2026 08 06.2246* 13 22 37.33 +53 41 48.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.15,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.19 13:19:16.02 +54:20:59.9
114.19522 62.30370 galactic UMa Second-epoch detections are separated by 1.6" and 0.9 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 | 13:19:16.02 +54:20:59.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.469+/-0.026 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:16.02 +54:20:59.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:16.02 +54:20:59.9: 13.15 +/- 0.03 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!
TCP 2026 08 06.2246* 13 19 16.02 +54 20 59.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.19,0.05,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 20260806.2246 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.14 13:19:57.74 +54:03:52.9
113.83639 62.55695 galactic UMa Second-epoch detections are separated by 2.7" and 0.5 pix
The object was found in VSX 1" Gaia DR3 1563622087226397824
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.810 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:57.74 +54:03:52.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:57.74 +54:03:52.9: 13.12 +/- 0.03 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!
TCP 2026 08 06.2246* 13 19 57.74 +54 03 52.9 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1563622087226397824,2461258.7246,12.14,0.05,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 1563622087226397824 20260806.2246 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 12.06 13:15:32.88 +54:54:05.9
115.57186 61.88074 galactic UMa Second-epoch detections are separated by 4.6" and 0.5 pix
The object was found in VSX 1" Gaia DR3 1564476506544266496
Type: ROT
# Max. Min./Amp. JD0 Period
12.690 G 12.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:32.88 +54:54:05.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:32.88 +54:54:05.9: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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!
TCP 2026 08 06.2246* 13 15 32.88 +54 54 05.9 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1564476506544266496,2461258.7246,12.06,0.05,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 1564476506544266496 20260806.2246 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.22 13:26:19.86 +54:59:31.7
112.45268 61.42050 galactic UMa Second-epoch detections are separated by 3.0" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:19.86 +54:59:31.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.328+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:26:19.86 +54:59:31.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:26:19.86 +54:59:31.7: 13.15 +/- 0.03 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!
TCP 2026 08 06.2246* 13 26 19.86 +54 59 31.7 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.22,0.05,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 20260806.2246 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.11 13:18:12.86 +55:26:54.2
115.02733 61.26702 galactic UMa Second-epoch detections are separated by 2.3" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:12.86 +55:26:54.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.357+/-0.030 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:18:12.86 +55:26:54.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:18:12.86 +55:26:54.2: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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!
TCP 2026 08 06.2246* 13 18 12.86 +55 26 54.2 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.11,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.16 13:26:11.86 +54:29:22.2
112.19095 61.90793 galactic UMa Second-epoch detections are separated by 2.4" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:11.86 +54:29:22.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.673+/-0.033 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:26:11.86 +54:29:22.2: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:26:11.86 +54:29:22.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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!
TCP 2026 08 06.2246* 13 26 11.86 +54 29 22.2 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.16,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.22 13:13:56.93 +55:25:59.0
116.25676 61.40249 galactic UMa Second-epoch detections are separated by 0.5" and 0.8 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 | 13:13:56.93 +55:25:59.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.357+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:13:56.93 +55:25:59.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:13:56.93 +55:25:59.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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!
TCP 2026 08 06.2246* 13 13 56.93 +55 25 59.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.22,0.05,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 20260806.2246 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.12 13:17:29.38 +53:16:42.3
114.21779 63.40684 galactic UMa Second-epoch detections are separated by 1.1" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J199.3728+53.2785 | 13:17:29.38 +53:16:42.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.505+/-0.031 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:29.38 +53:16:42.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:29.38 +53:16:42.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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!
TCP 2026 08 06.2246* 13 17 29.38 +53 16 42.3 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J199.3728+53.2785,2461258.7246,12.12,0.05,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
ATO J199.3728+53.2785 20260806.2246 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 06.2246 2461258.7246 12.06 13:14:45.50 +55:47:15.5
116.15931 61.03290 galactic UMa Second-epoch detections are separated by 0.5" and 0.9 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 | 13:14:45.50 +55:47:15.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.445+/-0.029 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:45.50 +55:47:15.5: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:45.50 +55:47:15.5: 13.02 +/- 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!
TCP 2026 08 06.2246* 13 14 45.50 +55 47 15.5 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.06,0.05,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 20260806.2246 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.11 13:16:08.97 +53:28:07.7
114.74537 63.26490 galactic UMa Second-epoch detections are separated by 1.3" and 0.5 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 J199.0371+53.4685 | 13:16:08.97 +53:28:07.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.411+/-0.032 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:08.97 +53:28:07.7: 13.07 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:08.97 +53:28:07.7: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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!
TCP 2026 08 06.2246* 13 16 08.97 +53 28 07.7 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J199.0371+53.4685,2461258.7246,12.11,0.05,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
ATO J199.0371+53.4685 20260806.2246 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 06.2246 2461258.7246 12.18 13:24:48.58 +55:47:30.1
113.33348 60.71031 galactic UMa Second-epoch detections are separated by 4.7" and 1.5 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 | 13:24:48.58 +55:47:30.1 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.034 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:48.58 +55:47:30.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:48.58 +55:47:30.1: 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!
TCP 2026 08 06.2246* 13 24 48.58 +55 47 30.1 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.18,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.04 13:19:11.73 +50:15:03.8
111.86119 66.27633 galactic CVn Second-epoch detections are separated by 2.3" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:11.73 +50:15:03.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.032 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:11.73 +50:15:03.8: 13.04 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:11.73 +50:15:03.8: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 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,2461258.7246,12.04,0.05,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 20260806.2246 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 06.2246 2461258.7246 11.96 13:20:49.90 +49:24:39.2
110.63011 67.00937 galactic CVn Second-epoch detections are separated by 0.6" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:49.90 +49:24:39.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.320+/-0.033 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:49.90 +49:24:39.2: 13.01 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:49.90 +49:24:39.2: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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,2461258.7246,11.96,0.05,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 20260806.2246 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 06.2246 2461258.7246 12.06 13:20:30.20 +48:49:37.7
110.31956 67.58320 galactic CVn Second-epoch detections are separated by 1.9" and 0.6 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 | 13:20:30.20 +48:49:37.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.369+/-0.035 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:30.20 +48:49:37.7: 13.01 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:30.20 +48:49:37.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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,2461258.7246,12.06,0.05,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 20260806.2246 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.11 13:15:03.01 +53:41:45.8
115.20349 63.07646 galactic UMa Second-epoch detections are separated by 1.5" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:03.01 +53:41:45.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.446+/-0.030 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:03.01 +53:41:45.8: 12.98 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:03.01 +53:41:45.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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!
TCP 2026 08 06.2246* 13 15 03.01 +53 41 45.8 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.11,0.05,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 20260806.2246 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 06.2246 2461258.7246 11.85 13:19:56.55 +49:16:33.2
110.88654 67.18036 galactic CVn Second-epoch detections are separated by 1.8" and 0.7 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 | 13:19:56.55 +49:16:33.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.402+/-0.031 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:56.55 +49:16:33.2: 13.00 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:56.55 +49:16:33.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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,2461258.7246,11.85,0.05,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 20260806.2246 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.09 13:11:27.42 +58:21:32.4
117.89650 58.57310 galactic UMa Second-epoch detections are separated by 1.4" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566657529592684928 | 13:11:27.40 +58:21:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:11:27.42 +58:21:32.4: 13.04 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:11:27.42 +58:21:32.4: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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!
TCP 2026 08 06.2246* 13 11 27.42 +58 21 32.4 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566657529592684928,2461258.7246,12.09,0.05,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
Gaia DR3 1566657529592684928 20260806.2246 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 06.2246 2461258.7246 11.94 13:16:16.88 +55:55:10.5
115.77964 60.86234 galactic UMa Second-epoch detections are separated by 1.4" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:16.88 +55:55:10.5 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:16.88 +55:55:10.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:16.88 +55:55:10.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 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!
TCP 2026 08 06.2246* 13 16 16.88 +55 55 10.5 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,11.94,0.05,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 20260806.2246 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 06.2246 2461258.7246 11.86 13:24:29.31 +54:14:53.6
112.55681 62.20925 galactic UMa Second-epoch detections are separated by 0.5" and 0.9 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 | 13:24:29.31 +54:14:53.6 (user input) | T | P | (position from user input) J-Ks=0.618+/-0.031 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:29.31 +54:14:53.6: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:29.31 +54:14:53.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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!
TCP 2026 08 06.2246* 13 24 29.31 +54 14 53.6 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,11.86,0.05,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 20260806.2246 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.98 13:19:56.20 +52:17:29.6
112.86592 64.27614 galactic CVn Second-epoch detections are separated by 3.5" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562872907491760000 | 13:19:56.62 +52:18:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.275+/-0.031 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:56.20 +52:17:29.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:56.20 +52:17:29.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562872907491760000,2461258.7246,11.98,0.05,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 1562872907491760000 20260806.2246 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 06.2246 2461258.7246 11.87 13:20:16.92 +50:05:25.9
111.33512 66.38325 galactic CVn Second-epoch detections are separated by 1.1" and 0.7 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 | 13:20:16.92 +50:05:25.9 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:16.92 +50:05:25.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:16.92 +50:05:25.9: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461258.7246,11.87,0.05,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 20260806.2246 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 06.2246 2461258.7246 11.90 13:23:08.24 +48:53:15.0
109.29115 67.39265 galactic CVn Second-epoch detections are separated by 4.2" and 0.7 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 | 13:23:08.24 +48:53:15.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:23:08.24 +48:53:15.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:23:08.24 +48:53:15.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461258.7246,11.90,0.05,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 20260806.2246 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.90 13:25:44.53 +53:56:26.7
111.99107 62.45278 galactic UMa Second-epoch detections are separated by 1.6" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:25:44.53 +53:56:26.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:25:44.53 +53:56:26.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:25:44.53 +53:56:26.7: 12.86 +/- 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!
TCP 2026 08 06.2246* 13 25 44.53 +53 56 26.7 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,11.90,0.05,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 20260806.2246 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.75 13:20:36.08 +50:12:06.6
111.29034 66.26208 galactic CVn Second-epoch detections are separated by 2.3" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:36.08 +50:12:06.6 (user input) | T | P | (position from user input) J-Ks=0.250+/-0.030 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:36.08 +50:12:06.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:36.08 +50:12:06.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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,2461258.7246,11.75,0.05,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 20260806.2246 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 11.76 13:22:46.96 +49:26:33.2
109.88164 66.88390 galactic CVn Second-epoch detections are separated by 1.8" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:46.96 +49:26:33.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.450+/-0.028 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:46.96 +49:26:33.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:46.96 +49:26:33.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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,2461258.7246,11.76,0.05,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 20260806.2246 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.68 13:21:55.08 +49:00:50.0
109.88789 67.33520 galactic CVn Second-epoch detections are separated by 1.1" and 0.8 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 | Large-amplitude variable Gaia DR2 1553144428608951808 | 13:21:55.08 +49:00:50.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.292+/-0.029 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:55.08 +49:00:50.0: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:55.08 +49:00:50.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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
Large-amplitude variable Gaia DR2 1553144428608951808,2461258.7246,11.68,0.05,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
Large-amplitude variable Gaia DR2 1553144428608951808 20260806.2246 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 06.2246 2461258.7246 11.59 13:19:41.82 +49:40:03.2
111.26649 66.81574 galactic CVn Second-epoch detections are separated by 1.3" and 0.9 pix
The object was found in VSX 1" Gaia DR3 1556181004847148032
Type: ROT
# Max. Min./Amp. JD0 Period
12.360 G 12.390 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:41.82 +49:40:03.2: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:41.82 +49:40:03.2: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 1556181004847148032,2461258.7246,11.59,0.05,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 1556181004847148032 20260806.2246 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 06.2246 2461258.7246 11.63 13:19:58.38 +49:40:23.6
111.16163 66.79783 galactic CVn Second-epoch detections are separated by 1.9" and 0.7 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 1553178753987511552 | 13:19:58.25 +49:40:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.259+/-0.032 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:58.38 +49:40:23.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:58.38 +49:40:23.6: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 1553178753987511552,2461258.7246,11.63,0.05,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 1553178753987511552 20260806.2246 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 06.2246 2461258.7246 11.50 13:19:59.47 +49:10:27.0
110.79183 67.27558 galactic CVn Second-epoch detections are separated by 1.1" and 0.8 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 1553139205928684288 | 13:19:59.52 +49:10:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.340+/-0.033 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:59.47 +49:10:27.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:59.47 +49:10:27.0: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 1553139205928684288,2461258.7246,11.50,0.05,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 1553139205928684288 20260806.2246 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.2246 2461258.7246 11.69 13:19:08.91 +49:48:12.0
111.57703 66.70954 galactic CVn Second-epoch detections are separated by 1.5" and 1.0 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 1556185952649445376 | 13:19:08.91 +49:48:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.493+/-0.032 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:08.91 +49:48:12.0: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:08.91 +49:48:12.0: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 1556185952649445376,2461258.7246,11.69,0.05,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
Gaia DR3 1556185952649445376 20260806.2246 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 06.2246 2461258.7246 11.54 13:20:38.03 +49:45:50.5
110.96731 66.68050 galactic CVn Second-epoch detections are separated by 1.2" and 0.8 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 | 13:20:38.03 +49:45:50.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.302+/-0.030 (F)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:38.03 +49:45:50.5: 12.42 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:38.03 +49:45:50.5: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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,2461258.7246,11.54,0.05,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 20260806.2246 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 11.45 13:20:59.03 +49:11:56.1
110.40929 67.20473 galactic CVn Second-epoch detections are separated by 1.7" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1553151536777926528 | 13:20:59.09 +49:11:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.394+/-0.034 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:59.03 +49:11:56.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:59.03 +49:11:56.1: 12.36 +/- 0.02 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 1553151536777926528,2461258.7246,11.45,0.05,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 1553151536777926528 20260806.2246 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 06.2246 2461258.7246 12.71 14:50:43.25 +51:16:27.1
88.08508 57.01172 galactic Boo Second-epoch detections are separated by 1.9" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J222.6772+51.2708 | 14:50:43.25 +51:16:27.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:50:43.25 +51:16:27.1: 13.84 +/- 0.06 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:50:43.25 +51:16:27.1: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 J222.6772+51.2708,2461258.7246,12.71,0.05,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 J222.6772+51.2708 20260806.2246 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.57 13:21:49.46 +55:12:48.3
113.87343 61.37720 galactic UMa Second-epoch detections are separated by 1.0" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:49.46 +55:12:48.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:49.46 +55:12:48.3: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:49.46 +55:12:48.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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!
TCP 2026 08 06.2246* 13 21 49.46 +55 12 48.3 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.57,0.05,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 20260806.2246 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2246 2461258.7246 12.50 13:13:04.66 +55:45:11.2
116.62706 61.10945 galactic UMa Second-epoch detections are separated by 3.4" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:04.66 +55:45:11.2 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.713+/-0.029 (K)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:13:04.66 +55:45:11.2: 13.68 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:13:04.66 +55:45:11.2: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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!
TCP 2026 08 06.2246* 13 13 04.66 +55 45 11.2 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7246,12.50,0.05,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 20260806.2246 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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: 2461176.78274846 16.05.2026 06:46:59.467 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
First image: 2461176.78274846 16.05.2026 06:46:59.467 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Last image: 2461258.72481094 06.08.2026 05:23:33.665 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 3 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): 6358
Objects passed selection criteria: 6331
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 4218.75
Average stars matched: 4129.75 (97.8904 %)
Memory usage VmPeak: 232736 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 00:26:46 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: 2461176.78274846 16.05.2026 06:46:59.467 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
First image: 2461176.78274846 16.05.2026 06:46:59.467 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Last image: 2461258.72481094 06.08.2026 05:23:33.665 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 152
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 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): 30653
Objects passed selection criteria: 30583
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 21904
Average stars matched: 21213 (96.8453 %)
Memory usage VmPeak: 254348 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 00:27:24 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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
SExtractor catalog cache: saved Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.cat to cache
SExtractor catalog cache: saved Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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: 2461258.72434925
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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits exists and is non-empty
Saving wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits to local_wcs_cache/
'wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits' -> 'local_wcs_cache/wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits'
wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits exists and is non-empty
Saving wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits to local_wcs_cache/
'wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits' -> 'local_wcs_cache/wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits'
wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits exists and is non-empty
Saving wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits to local_wcs_cache/
'wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits' -> 'local_wcs_cache/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits'
wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits exists and is non-empty
Saving wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits to local_wcs_cache/
'wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits' -> 'local_wcs_cache/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits (1st reference image)
verification OK: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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: 14:07:02.218 +54:00:47.22 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-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits (1st new image)
verification OK: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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: 14:07:13.958 +54:00:35.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:07:02.218 +54:00:47.22
Second-epoch image center 14:07:13.958 +54:00:35.47
Angular distance between the image centers 0.0289 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits (2nd new image)
verification OK: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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: 14:07:14.426 +54:00:38.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:07:02.218 +54:00:47.22
Second-epoch image center 14:07:14.426 +54:00:38.76
Angular distance between the image centers 0.0300 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 14:07:13.958 +54:00:35.47
Second-epoch second image center 14:07:14.426 +54:00:38.76
Angular distance between the image centers 0.00147 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00147 deg. (min. required shift: 0.00164 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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits &> /tmp/tmp.cLczClVUUB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits &> /tmp/tmp.CXxbp2jT5t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits &> /tmp/tmp.VHZKvAgrCK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits &> /tmp/tmp.TfD8SJ9dOz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
Found non-empty wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
The reference image (wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits) and catalog (wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat) found
'wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat' -> 'wcsmag.cat'
Read 6655 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.0728 to 226.7761 deg, Dec +48.2019 to +59.2571 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 197.0728 to 226.7761 deg, Dec 48.2019 to 59.2571 deg
Loaded 5155 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): 3600 out of 3709 total matches.
Matched with Tycho-2 3709 out of 6655 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.721600
a=0.000000 b=1.000000 c=22.721600
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6655 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.0728 to 226.7761 deg, Dec +48.2019 to +59.2571 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 197.0728 to 226.7761 deg, Dec 48.2019 to 59.2571 deg
Loaded 5155 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): 3600 out of 3709 total matches.
Matched with Tycho-2 3709 out of 6655 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Forced-photometry filter: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits -> calib.txt_param_ref_wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits (aperture=6.4)
Read 6628 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.0735 to 226.7760 deg, Dec +48.2020 to +59.2569 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 197.0735 to 226.7760 deg, Dec 48.2020 to 59.2569 deg
Loaded 5153 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): 3609 out of 3708 total matches.
Matched with Tycho-2 3708 out of 6628 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Forced-photometry filter: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits -> calib.txt_param_ref_wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
2.3 pix Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
2.6 pix fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
2.6 pix fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Limiting magnitude estimates:
15.3 mag. Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
15.3 mag. Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
12.8 mag. fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
12.8 mag. fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.6 (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.cLczClVUUB (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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits' -> 'wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Checking if the catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS catalog name: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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=399, bad_region=0, passed=6655
Got 6655 stars (including 6248 good ones) from the SExtractor catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
util/solve_plate_with_UCAC5 got 6655 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 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6655 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 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4892 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits N_match=4892 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.284 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.387 n_q1=1275 n_q2=1255 n_q3=1196 n_q4=1166 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits -region wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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.CXxbp2jT5t (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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits' -> 'wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Checking if the catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS catalog name: wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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=386, bad_region=0, passed=6628
Got 6628 stars (including 6234 good ones) from the SExtractor catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 6628 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 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 6628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 6628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 6628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits N_match=4895 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.379 n_q1=1274 n_q2=1261 n_q3=1200 n_q4=1160 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits -region wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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.VHZKvAgrCK (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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS_IMAGE_NAME=wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS-calibrated image found: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Checking if the catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS catalog name: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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=89, bad_region=0, passed=1847
Got 1847 stars (including 1751 good ones) from the SExtractor catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 1847 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 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 1710 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1710 matched stars entering correct_measured_positions(), 1709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1710 matched stars entering correct_measured_positions(), 1846 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 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 1710 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1710 matched stars entering correct_measured_positions(), 1846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 1710 matched stars entering correct_measured_positions(), 1846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 1710 stars left (next iteration limit 1881)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1710 robust_rms=9.805 arcsec worst_quadrant_rms=16.413 arcsec
SIP_REFIT: SIP order 3 trial: matched=1710 robust_rms=0.373 arcsec worst_quadrant_rms=0.399 arcsec
SIP_REFIT: SIP order 5 trial: matched=1710 robust_rms=0.300 arcsec worst_quadrant_rms=0.364 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1710 robust_rms_before=0.823 arcsec robust_rms_before_corrected=0.309 arcsec robust_rms_after=0.300 arcsec worst_quadrant_rms_before=0.348 worst_quadrant_rms_after=0.364
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.348 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits N_match=1710 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.308 sigma_q4_arcsec=0.276 n_q1=519 n_q2=383 n_q3=443 n_q4=365 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits -region wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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.TfD8SJ9dOz (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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS_IMAGE_NAME=wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS-calibrated image found: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Checking if the catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS catalog name: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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=89, bad_region=0, passed=1861
Got 1861 stars (including 1767 good ones) from the SExtractor catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 1861 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 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 1725 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1723 matched stars entering correct_measured_positions(), 1723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1723 matched stars entering correct_measured_positions(), 1861 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 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 1725 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1723 matched stars entering correct_measured_positions(), 1861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 1723 matched stars entering correct_measured_positions(), 1861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 1723 stars left (next iteration limit 1895)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1723 robust_rms=11.482 arcsec worst_quadrant_rms=13.754 arcsec
SIP_REFIT: SIP order 3 trial: matched=1723 robust_rms=0.382 arcsec worst_quadrant_rms=0.409 arcsec
SIP_REFIT: SIP order 5 trial: matched=1723 robust_rms=0.294 arcsec worst_quadrant_rms=0.363 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1723 robust_rms_before=0.821 arcsec robust_rms_before_corrected=0.315 arcsec robust_rms_after=0.294 arcsec worst_quadrant_rms_before=0.377 worst_quadrant_rms_after=0.363
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.377 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits N_match=1723 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.315 n_q1=507 n_q2=397 n_q3=428 n_q4=391 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits -region wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits sigma_overall=0.346 worst_q_ratio=1.116
ref2=Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits sigma_overall=0.366 worst_q_ratio=1.162
new1=fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits sigma_overall=0.308 worst_q_ratio=1.192
new2=fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits sigma_overall=0.324 worst_q_ratio=1.198
reference average sigma_overall=0.356 worst_q_ratio=1.139
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125_astrometric_residuals.png (4892 matched stars from wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126_astrometric_residuals.png (4895 matched stars from wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150_astrometric_residuals.png (1710 matched stars from wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151_astrometric_residuals.png (1723 matched stars from wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits'
Saving fully-calibrated image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits'
Preparing the HTML report for the field Boo-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:42:07.17 +49:07:36.2: 9.49 +/- 0.00 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:42:07.17 +49:07:36.2: 9.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.47 +/- 0.00
Forced photometry filter REJECTED candidate at 14:42:07.17 +49:07:36.2: ref_mag=9.47 +/- 0.00 new_mean_mag=10.0109 delta=-0.54 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20290_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 20290_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Boo-01-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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
SExtractor catalog cache: saved Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.cat to cache
SExtractor catalog cache: saved Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Creating symlink local_wcs_cache/wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits exists and is non-empty
wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits exists and is non-empty
wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits exists and is non-empty
wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits (1st reference image)
verification OK: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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: 14:07:02.218 +54:00:47.22 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-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits (1st new image)
verification OK: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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: 14:07:13.958 +54:00:35.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:07:02.218 +54:00:47.22
Second-epoch image center 14:07:13.958 +54:00:35.47
Angular distance between the image centers 0.0289 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits (2nd new image)
verification OK: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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: 14:07:14.426 +54:00:38.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:07:02.218 +54:00:47.22
Second-epoch image center 14:07:14.426 +54:00:38.76
Angular distance between the image centers 0.0300 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 14:07:13.958 +54:00:35.47
Second-epoch second image center 14:07:14.426 +54:00:38.76
Angular distance between the image centers 0.00147 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00147 deg. (min. required shift: 0.00164 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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits &> /tmp/tmp.29mf0ZggPr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits &> /tmp/tmp.8gKvO77Seu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits &> /tmp/tmp.OMSOJcVTr2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits &> /tmp/tmp.ppYwIPUzPC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
Found non-empty wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits and wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
The reference image (wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits) and catalog (wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat) found
'wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat' -> 'wcsmag.cat'
Read 32709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 196.9080 to 226.7761 deg, Dec +48.1413 to +59.2703 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 196.9080 to 226.7761 deg, Dec 48.1413 to 59.2703 deg
Loaded 5210 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): 3438 out of 3735 total matches.
Matched with Tycho-2 3735 out of 32709 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.620300
a=0.000000 b=1.000000 c=22.620300
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 32709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 196.9080 to 226.7761 deg, Dec +48.1413 to +59.2703 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 196.9080 to 226.7761 deg, Dec 48.1413 to 59.2703 deg
Loaded 5210 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): 3438 out of 3735 total matches.
Matched with Tycho-2 3735 out of 32709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Forced-photometry filter: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits -> calib.txt_param_ref_wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits (aperture=5.1)
Read 32853 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 196.9614 to 226.7760 deg, Dec +48.1376 to +59.2702 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 196.9614 to 226.7760 deg, Dec 48.1376 to 59.2702 deg
Loaded 5202 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): 3441 out of 3736 total matches.
Matched with Tycho-2 3736 out of 32853 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Forced-photometry filter: calibrated wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits -> calib.txt_param_ref_wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 132 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
2.2 pix Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
2.5 pix fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
2.5 pix fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Limiting magnitude estimates:
15.5 mag. Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
15.4 mag. Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
13.1 mag. fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
13.0 mag. fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.29mf0ZggPr (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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits' -> 'wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
Checking if the catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits
WCS catalog name: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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=18, blended=1435, bad_region=2, passed=32691
Got 32691 stars (including 31212 good ones) from the SExtractor catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat
util/solve_plate_with_UCAC5 got 32691 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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 4889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 32691 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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 32691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 32691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4889 stars left (next iteration limit 5377)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits N_match=4889 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.374 n_q1=1275 n_q2=1247 n_q3=1203 n_q4=1164 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits -region wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.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.8gKvO77Seu (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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits' -> 'wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
Checking if the catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits
WCS catalog name: wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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=15, blended=1500, bad_region=1, passed=32838
Got 32838 stars (including 31289 good ones) from the SExtractor catalog wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 32838 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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 32838 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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 32838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 32838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4892 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits N_match=4892 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.295 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.386 n_q1=1275 n_q2=1248 n_q3=1204 n_q4=1165 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits -region wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.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.OMSOJcVTr2 (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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS_IMAGE_NAME=wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS-calibrated image found: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Checking if the catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
WCS catalog name: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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=5, blended=207, bad_region=10, passed=11359
Got 11359 stars (including 11123 good ones) from the SExtractor catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat
util/solve_plate_with_UCAC5 got 11359 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 689 to 748 (Dec 47.8 to 59.4)
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: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 11359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 689 to 748 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 11359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 11359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4866 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits N_match=4866 sigma_overall_arcsec=0.442 sigma_q1_arcsec=0.418 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.464 n_q1=1527 n_q2=1080 n_q3=1231 n_q4=1028 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits -region wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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.ppYwIPUzPC (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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS_IMAGE_NAME=wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS-calibrated image found: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Checking if the catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
WCS catalog name: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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=182, bad_region=16, passed=11385
Got 11385 stars (including 11159 good ones) from the SExtractor catalog wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 11385 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 689 to 748 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 4859 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 11385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 689 to 748 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 11385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 11385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits N_match=4852 sigma_overall_arcsec=0.433 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.430 n_q1=1452 n_q2=1140 n_q3=1207 n_q4=1053 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Boo-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits -region wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-22-53_20.00sec_-0.00C_LIGHTs_0150.fits
Saving fully-calibrated image wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.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-01-Q1b1x1_002433_TTUQ1b1x1_321200_OF9LHEO6/wcs_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151.fits
Preparing the HTML report for the field Boo-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:30:03.26 +56:07:05.4: 10.92 +/- 0.00 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:42:04.22 +49:08:15.1: 12.47 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:06:14.32 +48:53:34.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:30:03.26 +56:07:05.4: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Forced photometry filter REJECTED candidate at 14:30:03.26 +56:07:05.4: ref_mag=10.90 +/- 0.00 new_mean_mag=11.0934 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:42:04.22 +49:08:15.1: 12.42 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:36:50.74 +56:24:10.7: 15.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 14:42:04.22 +49:08:15.1: ref_mag=12.44 +/- 0.01 new_mean_mag=12.3330 delta=0.11 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:06:14.32 +48:53:34.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:52:19.92 +56:35:58.8: 15.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 14:06:14.32 +48:53:34.3: ref_mag=12.65 +/- 0.01 new_mean_mag=12.2701 delta=0.38 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:05.39 +55:17:50.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:36:50.74 +56:24:10.7: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:52:19.92 +56:35:58.8: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:05.39 +55:17:50.1: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:25:00.92 +55:32:49.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:28.69 +53:50:13.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:38.48 +54:37:03.8: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:23:14.46 +54:05:55.4: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:54:05.90 +54:01:27.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:51:54.75 +51:47:00.2: 13.60 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:25:00.92 +55:32:49.9: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:19.92 +54:45:46.5: 13.53 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:28.69 +53:50:13.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:28.69 +53:50:13.8: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9590 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:38.48 +54:37:03.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:38.48 +54:37:03.8: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1644 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:23:14.46 +54:05:55.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 13:23:14.46 +54:05:55.4: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4334 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:54:05.90 +54:01:27.5: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 14:54:05.90 +54:01:27.5: ref_mag=13.46 +/- 0.03 new_mean_mag=12.5537 delta=0.91 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:51:54.75 +51:47:00.2: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 14:51:54.75 +51:47:00.2: ref_mag=13.57 +/- 0.03 new_mean_mag=12.5593 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:19.92 +54:45:46.5: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 13:19:19.92 +54:45:46.5: ref_mag=13.49 +/- 0.03 new_mean_mag=12.3840 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:57:06.97 +54:46:29.1: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:57:06.97 +54:46:29.1: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 14:57:06.97 +54:46:29.1: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6147 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:35.36 +55:29:52.6: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:35.36 +55:29:52.6: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 13:14:35.36 +55:29:52.6: ref_mag=13.53 +/- 0.03 new_mean_mag=12.3963 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:17.33 +54:55:06.5: 13.48 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:47.47 +49:08:16.4: 13.49 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:17.33 +54:55:06.5: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 13:19:17.33 +54:55:06.5: ref_mag=13.43 +/- 0.03 new_mean_mag=12.3728 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:47.47 +49:08:16.4: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 13:21:47.47 +49:08:16.4: ref_mag=13.51 +/- 0.03 new_mean_mag=12.2258 delta=1.28 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:36.73 +55:51:52.5: 13.44 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:24.69 +56:40:02.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:36.73 +55:51:52.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:36.73 +55:51:52.5: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3753 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:24.69 +56:40:02.0: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:24.69 +56:40:02.0: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3785 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:23.47 +54:20:09.7: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:23.47 +54:20:09.7: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 13:21:23.47 +54:20:09.7: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3556 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:38.77 +56:36:11.9: 13.40 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:15.37 +49:10:17.9: 13.37 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:38.77 +56:36:11.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:38.77 +56:36:11.9: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3991 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:15.37 +49:10:17.9: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 13:20:15.37 +49:10:17.9: ref_mag=13.36 +/- 0.03 new_mean_mag=12.1323 delta=1.23 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:27.54 +54:41:03.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:27.54 +54:41:03.9: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 13:21:27.54 +54:41:03.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2602 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:29:18.84 +54:46:28.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:29:18.84 +54:46:28.5: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 13:29:18.84 +54:46:28.5: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3484 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:07.02 +56:17:38.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:07.02 +56:17:38.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 13:17:07.02 +56:17:38.8: ref_mag=13.33 +/- 0.02 new_mean_mag=12.3393 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:49:19.07 +53:57:26.8: 13.33 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:49:19.07 +53:57:26.8: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 13:49:19.07 +53:57:26.8: ref_mag=13.34 +/- 0.02 new_mean_mag=12.4153 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:25.92 +52:52:38.0: 13.29 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:03.48 +53:43:25.6: 13.30 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:25.92 +52:52:38.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:52.15 +57:21:53.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 13:22:25.92 +52:52:38.0: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2702 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:03.48 +53:43:25.6: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:03.48 +53:43:25.6: ref_mag=13.30 +/- 0.02 new_mean_mag=12.1795 delta=1.12 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:05.05 +55:07:28.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:52.15 +57:21:53.6: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 13:15:52.15 +57:21:53.6: ref_mag=13.22 +/- 0.02 new_mean_mag=12.3686 delta=0.85 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:05.05 +55:07:28.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 13:17:05.05 +55:07:28.8: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3042 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:53.49 +52:06:03.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:58.55 +49:27:41.4: 13.26 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:53.49 +52:06:03.7: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 13:17:53.49 +52:06:03.7: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1458 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:58.55 +49:27:41.4: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:58.55 +49:27:41.4: ref_mag=13.23 +/- 0.02 new_mean_mag=12.0189 delta=1.21 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:24.39 +50:07:43.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:17.94 +49:38:30.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:24.39 +50:07:43.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:24.39 +50:07:43.8: ref_mag=13.27 +/- 0.02 new_mean_mag=12.0918 delta=1.18 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:17.94 +49:38:30.1: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 13:20:17.94 +49:38:30.1: ref_mag=13.31 +/- 0.03 new_mean_mag=12.0039 delta=1.30 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:53.28 +49:24:13.3: 13.27 +/- 0.04 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:24.05 +55:27:09.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:53.28 +49:24:13.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:53.28 +49:24:13.3: ref_mag=13.24 +/- 0.02 new_mean_mag=12.0057 delta=1.24 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:24.05 +55:27:09.5: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 13:16:24.05 +55:27:09.5: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2323 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:39.24 +50:06:34.2: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:39.24 +50:06:34.2: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:39.24 +50:06:34.2: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2422 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:26.24 +55:08:38.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:26.24 +55:08:38.4: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 13:24:26.24 +55:08:38.4: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2929 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:46.90 +49:15:28.3: 13.17 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:12.90 +49:51:22.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:23.43 +56:10:13.7: 13.21 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:46.90 +49:15:28.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:12.90 +49:51:22.8: 13.20 +/- 0.03 detection
Forced photometry filter KEPT candidate at 13:20:46.90 +49:15:28.3: ref_mag=13.18 +/- 0.02 new_mean_mag=11.9865 delta=1.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:12.90 +49:51:22.8: ref_mag=13.21 +/- 0.02 new_mean_mag=12.0820 delta=1.13 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:23.43 +56:10:13.7: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 13:17:23.43 +56:10:13.7: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1574 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:10.48 +49:23:34.4: 13.17 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:10.48 +49:23:34.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:10.48 +49:23:34.4: ref_mag=13.12 +/- 0.02 new_mean_mag=12.0752 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:18:09.50 +56:50:49.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:37.33 +53:41:48.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:18:09.50 +56:50:49.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 13:18:09.50 +56:50:49.0: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2372 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:37.33 +53:41:48.0: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 13:22:37.33 +53:41:48.0: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1585 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:16.02 +54:20:59.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:57.74 +54:03:52.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:26:19.86 +54:59:31.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:32.88 +54:54:05.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:16.02 +54:20:59.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:57.74 +54:03:52.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:16.02 +54:20:59.9: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1899 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 13:19:57.74 +54:03:52.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1369 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:26:19.86 +54:59:31.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:32.88 +54:54:05.9: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 13:26:19.86 +54:59:31.7: ref_mag=13.15 +/- 0.02 new_mean_mag=12.2146 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 13:15:32.88 +54:54:05.9: ref_mag=13.16 +/- 0.02 new_mean_mag=12.0635 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:18:12.86 +55:26:54.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:18:12.86 +55:26:54.2: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 13:18:12.86 +55:26:54.2: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0936 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:26:11.86 +54:29:22.2: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:13:56.93 +55:25:59.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:26:11.86 +54:29:22.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 13:26:11.86 +54:29:22.2: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1482 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:13:56.93 +55:25:59.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:56.93 +55:25:59.0: ref_mag=13.16 +/- 0.02 new_mean_mag=12.2045 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:17:29.38 +53:16:42.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:17:29.38 +53:16:42.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 13:17:29.38 +53:16:42.3: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1113 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:45.50 +55:47:15.5: 13.11 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:45.50 +55:47:15.5: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:45.50 +55:47:15.5: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0654 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:08.97 +53:28:07.7: 13.07 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:08.97 +53:28:07.7: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 13:16:08.97 +53:28:07.7: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1022 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:48.58 +55:47:30.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:11.73 +50:15:03.8: 13.04 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:48.58 +55:47:30.1: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:11.73 +50:15:03.8: 13.02 +/- 0.03 detection
Forced photometry filter KEPT candidate at 13:24:48.58 +55:47:30.1: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1499 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:11.73 +50:15:03.8: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9717 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:49.90 +49:24:39.2: 13.01 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:30.20 +48:49:37.7: 13.01 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:49.90 +49:24:39.2: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:49.90 +49:24:39.2: ref_mag=13.01 +/- 0.02 new_mean_mag=11.9241 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:30.20 +48:49:37.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:30.20 +48:49:37.7: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0405 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:15:03.01 +53:41:45.8: 12.98 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:15:03.01 +53:41:45.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:03.01 +53:41:45.8: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0269 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:56.55 +49:16:33.2: 13.00 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:11:27.42 +58:21:32.4: 13.04 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:56.55 +49:16:33.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:56.55 +49:16:33.2: ref_mag=13.01 +/- 0.02 new_mean_mag=11.8349 delta=1.17 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:11:27.42 +58:21:32.4: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 13:11:27.42 +58:21:32.4: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0685 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:16:16.88 +55:55:10.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:16:16.88 +55:55:10.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 13:16:16.88 +55:55:10.5: ref_mag=12.98 +/- 0.02 new_mean_mag=11.9357 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:14:14.43 +56:16:08.8: 12.93 +/- 0.03 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:14:14.43 +56:16:08.8: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 13:14:14.43 +56:16:08.8: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0664 delta=0.90 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:24:29.31 +54:14:53.6: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:56.20 +52:17:29.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:24:29.31 +54:14:53.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 13:24:29.31 +54:14:53.6: ref_mag=12.87 +/- 0.01 new_mean_mag=11.8564 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:56.20 +52:17:29.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:56.20 +52:17:29.6: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9734 delta=0.90 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:16.92 +50:05:25.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:23:08.24 +48:53:15.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:16.92 +50:05:25.9: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:16.92 +50:05:25.9: ref_mag=12.85 +/- 0.02 new_mean_mag=11.8476 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:23:08.24 +48:53:15.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 13:23:08.24 +48:53:15.0: ref_mag=12.83 +/- 0.02 new_mean_mag=11.8942 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:25:44.53 +53:56:26.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:36.08 +50:12:06.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:25:44.53 +53:56:26.7: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 13:25:44.53 +53:56:26.7: ref_mag=12.82 +/- 0.01 new_mean_mag=11.9031 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:36.08 +50:12:06.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 13:20:36.08 +50:12:06.6: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7420 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:11:50.42 +57:07:30.6: 12.44 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:11:50.42 +57:07:30.6: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 13:11:50.42 +57:07:30.6: ref_mag=12.41 +/- 0.01 new_mean_mag=11.6212 delta=0.79 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:22:46.96 +49:26:33.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:55.08 +49:00:50.0: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:41.82 +49:40:03.2: 12.65 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:22:46.96 +49:26:33.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter KEPT candidate at 13:22:46.96 +49:26:33.2: ref_mag=12.75 +/- 0.02 new_mean_mag=11.7222 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:55.08 +49:00:50.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 13:21:55.08 +49:00:50.0: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6708 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:41.82 +49:40:03.2: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 13:19:41.82 +49:40:03.2: ref_mag=12.64 +/- 0.01 new_mean_mag=11.5763 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:58.38 +49:40:23.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:58.38 +49:40:23.6: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 13:19:58.38 +49:40:23.6: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6351 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:59.47 +49:10:27.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:59.47 +49:10:27.0: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 13:19:59.47 +49:10:27.0: ref_mag=12.60 +/- 0.01 new_mean_mag=11.4989 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:19:08.91 +49:48:12.0: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:38.03 +49:45:50.5: 12.42 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:38.03 +49:45:50.5: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:19:08.91 +49:48:12.0: 12.65 +/- 0.02 detection
Forced photometry filter KEPT candidate at 13:20:38.03 +49:45:50.5: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4638 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 13:19:08.91 +49:48:12.0: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6844 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:20:59.03 +49:11:56.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 14:50:43.25 +51:16:27.1: 13.84 +/- 0.06 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:20:59.03 +49:11:56.1: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 13:20:59.03 +49:11:56.1: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4312 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 14:50:43.25 +51:16:27.1: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 14:50:43.25 +51:16:27.1: ref_mag=13.86 +/- 0.04 new_mean_mag=12.7177 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:21:49.46 +55:12:48.3: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-46-59_20.00sec_-0.00C_LIGHT_0125.fits at 13:13:04.66 +55:45:11.2: 13.68 +/- 0.05 detection
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:21:49.46 +55:12:48.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 13:21:49.46 +55:12:48.3: ref_mag=13.73 +/- 0.03 new_mean_mag=12.5643 delta=1.16 (need > 0.90)
Forced photometry on wcs_Boo-01-Q1b1x1_2026-05-16_01-47-41_20.00sec_-0.00C_LIGHT_0126.fits at 13:13:04.66 +55:45:11.2: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 13:13:04.66 +55:45:11.2: ref_mag=13.69 +/- 0.03 new_mean_mag=12.4891 delta=1.20 (need > 0.90)
Adding exclusion_list_local.txt__out00667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52703.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 92s
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: 39s
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Considering the candidate 52314_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52314_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
**** FOUND 14:26:24.09 +57:45:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52316_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52316_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 52340_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52340_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52344_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52344_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52347_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52347_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52363_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52363_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52373_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52373_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52389_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52389_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52393_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52393_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52401_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52401_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52405_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52405_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52418_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52418_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52432_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52432_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52434_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52434_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52436_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52436_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52448_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52448_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
**** FOUND 14:15:48.88 +56:40:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52458_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52458_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52468_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52468_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52470_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52470_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52483_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52483_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52491_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52491_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52509_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52509_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52525_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52525_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52527_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52527_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52543_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52543_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52548_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52548_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 52552_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52552_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52553_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52553_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52577_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52577_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 52580_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52580_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52583_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52583_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52587_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52587_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52592_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52592_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52595_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52595_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52605_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52605_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52608_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52608_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52623_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52623_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52631_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52631_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52640_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52640_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52649_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52649_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52654_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 52654_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 52657_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52657_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52660_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52660_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52669_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52669_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52672_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52672_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52677_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52677_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52679_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 52679_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 52684_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52684_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52685_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 52685_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 52690_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52690_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52692_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52692_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52693_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52693_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52696_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52696_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52702_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 52702_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52703_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 52703_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 15265_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 15265_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 12697_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 12697_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 15014_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 15014_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26576_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26576_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 14581_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 14581_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 12601_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 12601_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 11824_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 11824_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 09714_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 09714_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 12063_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 12063_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 22525_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 22525_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 09005_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 09005_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 06256_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 06256_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 14124_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 14124_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 06539_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 06539_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23543_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23543_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 12961_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 12961_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 13191_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 13191_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 07269_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 07269_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 16734_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 16734_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 19042_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 19042_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 15607_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 15607_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 03897_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 03897_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 11140_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 11140_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 24112_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24112_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 24511_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24511_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26786_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26786_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 25301_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 25301_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 24339_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24339_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 10002_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 10002_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26802_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26802_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 11652_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 11652_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26114_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26114_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23962_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23962_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 07761_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 07761_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 24423_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24423_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 05628_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 05628_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 16268_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 16268_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 13900_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 13900_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 14893_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 14893_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 11779_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 11779_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 12300_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 12300_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 10146_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 10146_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 13928_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 13928_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 09877_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 09877_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 17242_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 17242_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 08786_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 08786_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 16512_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 16512_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 09526_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 09526_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 27373_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 27373_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 24513_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24513_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 21699_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 21699_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 15640_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 15640_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23727_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23727_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 00667_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 00667_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 08499_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 08499_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 07098_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 07098_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 22742_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 22742_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 14631_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 14631_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23041_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23041_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26549_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26549_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 21703_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 21703_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 15691_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 15691_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26891_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26891_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 04270_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 04270_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
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Considering the candidate 25549_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 25549_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
**** FOUND 13:57:47.52 +50:09:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24397_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 24397_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 22145_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 22145_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 25528_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 25528_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 25545_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 25545_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23750_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23750_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 26014_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 26014_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 25724_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 25724_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 23694_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 23694_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 29558_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 29558_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 11232_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 11232_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 08779_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
Preparing report for the candidate 08779_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
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Considering the candidate 11571_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151
The candidate 11571_fd_Boo-01-Q1b1x1_2026-08-06_00-23-33_20.00sec_0.00C_LIGHTs_0151 did not pass the final checks
**** FOUND 13:23:56.40 +54:55:30.9 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 136s
Prepared the HTML report for the field Boo-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:11:27.42 +58:21:32.4
13:18:09.50 +56:50:49.0
13:19:24.69 +56:40:02.0
13:20:38.77 +56:36:11.9
13:17:07.02 +56:17:38.8
13:17:23.43 +56:10:13.7
13:16:16.88 +55:55:10.5
13:13:04.66 +55:45:11.2
13:14:45.50 +55:47:15.5
13:20:36.73 +55:51:52.5
13:24:48.58 +55:47:30.1
13:14:35.36 +55:29:52.6
13:13:56.93 +55:25:59.0
13:16:24.05 +55:27:09.5
13:18:12.86 +55:26:54.2
13:17:05.05 +55:07:28.8
13:21:49.46 +55:12:48.3
13:24:26.24 +55:08:38.4
13:15:32.88 +54:54:05.9
14:57:06.97 +54:46:29.1
13:19:17.33 +54:55:06.5
13:26:19.86 +54:59:31.7
13:19:19.92 +54:45:46.5
13:14:38.48 +54:37:03.8
13:21:27.54 +54:41:03.9
13:29:18.84 +54:46:28.5
13:19:16.02 +54:20:59.9
13:26:11.86 +54:29:22.2
13:21:23.47 +54:20:09.7
14:54:05.90 +54:01:27.5
13:24:29.31 +54:14:53.6
13:19:57.74 +54:03:52.9
13:23:14.46 +54:05:55.4
13:15:28.69 +53:50:13.8
13:15:03.48 +53:43:25.6
13:15:03.01 +53:41:45.8
13:25:44.53 +53:56:26.7
13:22:37.33 +53:41:48.0
13:16:08.97 +53:28:07.7
13:49:19.07 +53:57:26.8
13:17:29.38 +53:16:42.3
13:22:25.92 +52:52:38.0
13:20:30.20 +48:49:37.7
13:23:08.24 +48:53:15.0
13:21:55.08 +49:00:50.0
13:21:47.47 +49:08:16.4
13:19:56.20 +52:17:29.6
13:20:15.37 +49:10:17.9
13:20:59.03 +49:11:56.1
13:19:56.55 +49:16:33.2
13:19:59.47 +49:10:27.0
13:20:46.90 +49:15:28.3
13:17:53.49 +52:06:03.7
13:19:53.28 +49:24:13.3
13:22:46.96 +49:26:33.2
13:20:10.48 +49:23:34.4
13:19:58.55 +49:27:41.4
13:20:49.90 +49:24:39.2
13:20:17.94 +49:38:30.1
13:19:41.82 +49:40:03.2
13:19:58.38 +49:40:23.6
13:20:38.03 +49:45:50.5
13:19:08.91 +49:48:12.0
13:20:12.90 +49:51:22.8
13:20:16.92 +50:05:25.9
14:51:54.75 +51:47:00.2
13:20:24.39 +50:07:43.8
13:20:39.24 +50:06:34.2
13:20:36.08 +50:12:06.6
13:19:11.73 +50:15:03.8
14:50:43.25 +51:16:27.1
13:36:50.74 +56:24:10.7
14:52:19.92 +56:35:58.8
13:17:05.39 +55:17:50.1
14:25:00.92 +55:32:49.9
########### Completed Boo-01-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 ####
13:36:50.74 +56:24:10.7
14:52:19.92 +56:35:58.8
13:17:05.39 +55:17:50.1
14:25:00.92 +55:32:49.9
13:15:28.69 +53:50:13.8
13:14:38.48 +54:37:03.8
13:23:14.46 +54:05:55.4
14:51:54.75 +51:47:00.2
14:54:05.90 +54:01:27.5
13:19:19.92 +54:45:46.5
14:57:06.97 +54:46:29.1
13:14:35.36 +55:29:52.6
13:19:17.33 +54:55:06.5
13:21:47.47 +49:08:16.4
13:20:36.73 +55:51:52.5
13:19:24.69 +56:40:02.0
13:21:23.47 +54:20:09.7
13:20:38.77 +56:36:11.9
13:20:15.37 +49:10:17.9
13:21:27.54 +54:41:03.9
13:29:18.84 +54:46:28.5
13:17:07.02 +56:17:38.8
13:49:19.07 +53:57:26.8
13:22:25.92 +52:52:38.0
13:15:03.48 +53:43:25.6
13:17:05.05 +55:07:28.8
13:17:53.49 +52:06:03.7
13:19:58.55 +49:27:41.4
13:20:24.39 +50:07:43.8
13:20:17.94 +49:38:30.1
13:19:53.28 +49:24:13.3
13:16:24.05 +55:27:09.5
13:20:39.24 +50:06:34.2
13:24:26.24 +55:08:38.4
13:20:12.90 +49:51:22.8
13:20:46.90 +49:15:28.3
13:17:23.43 +56:10:13.7
13:20:10.48 +49:23:34.4
13:18:09.50 +56:50:49.0
13:22:37.33 +53:41:48.0
13:19:16.02 +54:20:59.9
13:19:57.74 +54:03:52.9
13:15:32.88 +54:54:05.9
13:26:19.86 +54:59:31.7
13:18:12.86 +55:26:54.2
13:26:11.86 +54:29:22.2
13:13:56.93 +55:25:59.0
13:17:29.38 +53:16:42.3
13:14:45.50 +55:47:15.5
13:16:08.97 +53:28:07.7
13:24:48.58 +55:47:30.1
13:19:11.73 +50:15:03.8
13:20:49.90 +49:24:39.2
13:20:30.20 +48:49:37.7
13:15:03.01 +53:41:45.8
13:19:56.55 +49:16:33.2
13:11:27.42 +58:21:32.4
13:16:16.88 +55:55:10.5
13:24:29.31 +54:14:53.6
13:19:56.20 +52:17:29.6
13:20:16.92 +50:05:25.9
13:23:08.24 +48:53:15.0
13:25:44.53 +53:56:26.7
13:20:36.08 +50:12:06.6
13:22:46.96 +49:26:33.2
13:21:55.08 +49:00:50.0
13:19:41.82 +49:40:03.2
13:19:58.38 +49:40:23.6
13:19:59.47 +49:10:27.0
13:19:08.91 +49:48:12.0
13:20:38.03 +49:45:50.5
13:20:59.03 +49:11:56.1
14:50:43.25 +51:16:27.1
13:21:49.46 +55:12:48.3
13:13:04.66 +55:45:11.2
###################################################################################
13:36:50.74 +56:24:10.7 -- not an asteroid (will add it to exclusion list)
14:52:19.92 +56:35:58.8 -- not an asteroid (will add it to exclusion list)
13:17:05.39 +55:17:50.1 -- not an asteroid (will add it to exclusion list)
14:25:00.92 +55:32:49.9 -- not an asteroid (will add it to exclusion list)
13:15:28.69 +53:50:13.8 -- not an asteroid (will add it to exclusion list)
13:14:38.48 +54:37:03.8 -- not an asteroid (will add it to exclusion list)
13:23:14.46 +54:05:55.4 -- not an asteroid (will add it to exclusion list)
14:51:54.75 +51:47:00.2 -- not an asteroid (will add it to exclusion list)
14:54:05.90 +54:01:27.5 -- not an asteroid (will add it to exclusion list)
13:19:19.92 +54:45:46.5 -- not an asteroid (will add it to exclusion list)
14:57:06.97 +54:46:29.1 -- not an asteroid (will add it to exclusion list)
13:14:35.36 +55:29:52.6 -- not an asteroid (will add it to exclusion list)
13:19:17.33 +54:55:06.5 -- not an asteroid (will add it to exclusion list)
13:21:47.47 +49:08:16.4 -- not an asteroid (will add it to exclusion list)
13:20:36.73 +55:51:52.5 -- not an asteroid (will add it to exclusion list)
13:19:24.69 +56:40:02.0 -- not an asteroid (will add it to exclusion list)
13:21:23.47 +54:20:09.7 -- not an asteroid (will add it to exclusion list)
13:20:38.77 +56:36:11.9 -- not an asteroid (will add it to exclusion list)
13:20:15.37 +49:10:17.9 -- not an asteroid (will add it to exclusion list)
13:21:27.54 +54:41:03.9 -- not an asteroid (will add it to exclusion list)
13:29:18.84 +54:46:28.5 -- not an asteroid (will add it to exclusion list)
13:17:07.02 +56:17:38.8 -- not an asteroid (will add it to exclusion list)
13:49:19.07 +53:57:26.8 -- not an asteroid (will add it to exclusion list)
13:22:25.92 +52:52:38.0 -- not an asteroid (will add it to exclusion list)
13:15:03.48 +53:43:25.6 -- not an asteroid (will add it to exclusion list)
13:17:05.05 +55:07:28.8 -- not an asteroid (will add it to exclusion list)
13:17:53.49 +52:06:03.7 -- not an asteroid (will add it to exclusion list)
13:19:58.55 +49:27:41.4 -- not an asteroid (will add it to exclusion list)
13:20:24.39 +50:07:43.8 -- not an asteroid (will add it to exclusion list)
13:20:17.94 +49:38:30.1 -- not an asteroid (will add it to exclusion list)
13:19:53.28 +49:24:13.3 -- not an asteroid (will add it to exclusion list)
13:16:24.05 +55:27:09.5 -- not an asteroid (will add it to exclusion list)
13:20:39.24 +50:06:34.2 -- not an asteroid (will add it to exclusion list)
13:24:26.24 +55:08:38.4 -- not an asteroid (will add it to exclusion list)
13:20:12.90 +49:51:22.8 -- not an asteroid (will add it to exclusion list)
13:20:46.90 +49:15:28.3 -- not an asteroid (will add it to exclusion list)
13:17:23.43 +56:10:13.7 -- not an asteroid (will add it to exclusion list)
13:20:10.48 +49:23:34.4 -- not an asteroid (will add it to exclusion list)
13:18:09.50 +56:50:49.0 -- not an asteroid (will add it to exclusion list)
13:22:37.33 +53:41:48.0 -- not an asteroid (will add it to exclusion list)
13:19:16.02 +54:20:59.9 -- not an asteroid (will add it to exclusion list)
13:19:57.74 +54:03:52.9 -- not an asteroid (will add it to exclusion list)
13:15:32.88 +54:54:05.9 -- not an asteroid (will add it to exclusion list)
13:26:19.86 +54:59:31.7 -- not an asteroid (will add it to exclusion list)
13:18:12.86 +55:26:54.2 -- not an asteroid (will add it to exclusion list)
13:26:11.86 +54:29:22.2 -- not an asteroid (will add it to exclusion list)
13:13:56.93 +55:25:59.0 -- not an asteroid (will add it to exclusion list)
13:17:29.38 +53:16:42.3 -- not an asteroid (will add it to exclusion list)
13:14:45.50 +55:47:15.5 -- not an asteroid (will add it to exclusion list)
13:16:08.97 +53:28:07.7 -- not an asteroid (will add it to exclusion list)
13:24:48.58 +55:47:30.1 -- not an asteroid (will add it to exclusion list)
13:19:11.73 +50:15:03.8 -- not an asteroid (will add it to exclusion list)
13:20:49.90 +49:24:39.2 -- not an asteroid (will add it to exclusion list)
13:20:30.20 +48:49:37.7 -- not an asteroid (will add it to exclusion list)
13:15:03.01 +53:41:45.8 -- not an asteroid (will add it to exclusion list)
13:19:56.55 +49:16:33.2 -- not an asteroid (will add it to exclusion list)
13:11:27.42 +58:21:32.4 -- not an asteroid (will add it to exclusion list)
13:16:16.88 +55:55:10.5 -- not an asteroid (will add it to exclusion list)
13:24:29.31 +54:14:53.6 -- not an asteroid (will add it to exclusion list)
13:19:56.20 +52:17:29.6 -- not an asteroid (will add it to exclusion list)
13:20:16.92 +50:05:25.9 -- not an asteroid (will add it to exclusion list)
13:23:08.24 +48:53:15.0 -- not an asteroid (will add it to exclusion list)
13:25:44.53 +53:56:26.7 -- not an asteroid (will add it to exclusion list)
13:20:36.08 +50:12:06.6 -- not an asteroid (will add it to exclusion list)
13:22:46.96 +49:26:33.2 -- not an asteroid (will add it to exclusion list)
13:21:55.08 +49:00:50.0 -- not an asteroid (will add it to exclusion list)
13:19:41.82 +49:40:03.2 -- not an asteroid (will add it to exclusion list)
13:19:58.38 +49:40:23.6 -- not an asteroid (will add it to exclusion list)
13:19:59.47 +49:10:27.0 -- not an asteroid (will add it to exclusion list)
13:19:08.91 +49:48:12.0 -- not an asteroid (will add it to exclusion list)
13:20:38.03 +49:45:50.5 -- not an asteroid (will add it to exclusion list)
13:20:59.03 +49:11:56.1 -- not an asteroid (will add it to exclusion list)
14:50:43.25 +51:16:27.1 -- not an asteroid (will add it to exclusion list)
13:21:49.46 +55:12:48.3 -- not an asteroid (will add it to exclusion list)
13:13:04.66 +55:45:11.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
13:11:27.42 +58:21:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:04.66 +55:45:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:56.93 +55:25:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:35.36 +55:29:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:38.48 +54:37:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:45.50 +55:47:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:03.01 +53:41:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:03.48 +53:43:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:28.69 +53:50:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:32.88 +54:54:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:08.97 +53:28:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:16.88 +55:55:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:24.05 +55:27:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:05.05 +55:07:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:05.39 +55:17:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:07.02 +56:17:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:23.43 +56:10:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:29.38 +53:16:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:53.49 +52:06:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:09.50 +56:50:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:12.86 +55:26:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:08.91 +49:48:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:11.73 +50:15:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:16.02 +54:20:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:17.33 +54:55:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:19.92 +54:45:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:24.69 +56:40:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:41.82 +49:40:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:53.28 +49:24:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:56.20 +52:17:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:56.55 +49:16:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:57.74 +54:03:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:58.38 +49:40:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:58.55 +49:27:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:59.47 +49:10:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:10.48 +49:23:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:12.90 +49:51:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:15.37 +49:10:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:16.92 +50:05:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:17.94 +49:38:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:24.39 +50:07:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:30.20 +48:49:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:36.08 +50:12:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:36.73 +55:51:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:38.03 +49:45:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:38.77 +56:36:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:39.24 +50:06:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:46.90 +49:15:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:49.90 +49:24:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:59.03 +49:11:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:23.47 +54:20:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:27.54 +54:41:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:47.47 +49:08:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:49.46 +55:12:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:55.08 +49:00:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:25.92 +52:52:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:37.33 +53:41:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:46.96 +49:26:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:08.24 +48:53:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:14.46 +54:05:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:26.24 +55:08:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:29.31 +54:14:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:48.58 +55:47:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:44.53 +53:56:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:11.86 +54:29:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:19.86 +54:59:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:18.84 +54:46:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:50.74 +56:24:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:49:19.07 +53:57:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:25:00.92 +55:32:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:43.25 +51:16:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:51:54.75 +51:47:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:52:19.92 +56:35:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:05.90 +54:01:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:57:06.97 +54:46:29.1 -- 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)
13:11:27.42 +58:21:32.4 -- not a known variable star
13:13:04.66 +55:45:11.2 -- not a known variable star
13:13:56.93 +55:25:59.0 -- not a known variable star
13:14:35.36 +55:29:52.6 -- not a known variable star
13:14:38.48 +54:37:03.8 -- not a known variable star
13:14:45.50 +55:47:15.5 -- not a known variable star
13:15:03.01 +53:41:45.8 -- not a known variable star
13:15:03.48 +53:43:25.6 -- not a known variable star
13:15:28.69 +53:50:13.8 -- not a known variable star
13:15:32.88 +54:54:05.9 -- a known variable star
13:16:08.97 +53:28:07.7 -- not a known variable star
13:16:16.88 +55:55:10.5 -- not a known variable star
13:16:24.05 +55:27:09.5 -- not a known variable star
13:17:05.05 +55:07:28.8 -- not a known variable star
13:17:05.39 +55:17:50.1 -- not a known variable star
13:17:07.02 +56:17:38.8 -- a known variable star
13:17:23.43 +56:10:13.7 -- a known variable star
13:17:29.38 +53:16:42.3 -- not a known variable star
13:17:53.49 +52:06:03.7 -- a known variable star
13:18:09.50 +56:50:49.0 -- not a known variable star
13:18:12.86 +55:26:54.2 -- not a known variable star
13:19:08.91 +49:48:12.0 -- not a known variable star
13:19:11.73 +50:15:03.8 -- not a known variable star
13:19:16.02 +54:20:59.9 -- not a known variable star
13:19:17.33 +54:55:06.5 -- not a known variable star
13:19:19.92 +54:45:46.5 -- not a known variable star
13:19:24.69 +56:40:02.0 -- not a known variable star
13:19:41.82 +49:40:03.2 -- a known variable star
13:19:53.28 +49:24:13.3 -- not a known variable star
13:19:56.20 +52:17:29.6 -- not a known variable star
13:19:56.55 +49:16:33.2 -- not a known variable star
13:19:57.74 +54:03:52.9 -- a known variable star
13:19:58.38 +49:40:23.6 -- not a known variable star
13:19:58.55 +49:27:41.4 -- not a known variable star
13:19:59.47 +49:10:27.0 -- not a known variable star
13:20:10.48 +49:23:34.4 -- not a known variable star
13:20:12.90 +49:51:22.8 -- not a known variable star
13:20:15.37 +49:10:17.9 -- not a known variable star
13:20:16.92 +50:05:25.9 -- not a known variable star
13:20:17.94 +49:38:30.1 -- not a known variable star
13:20:24.39 +50:07:43.8 -- not a known variable star
13:20:30.20 +48:49:37.7 -- not a known variable star
13:20:36.08 +50:12:06.6 -- not a known variable star
13:20:36.73 +55:51:52.5 -- not a known variable star
13:20:38.03 +49:45:50.5 -- not a known variable star
13:20:38.77 +56:36:11.9 -- not a known variable star
13:20:39.24 +50:06:34.2 -- not a known variable star
13:20:46.90 +49:15:28.3 -- a known variable star
13:20:49.90 +49:24:39.2 -- not a known variable star
13:20:59.03 +49:11:56.1 -- not a known variable star
13:21:23.47 +54:20:09.7 -- not a known variable star
13:21:27.54 +54:41:03.9 -- not a known variable star
13:21:47.47 +49:08:16.4 -- not a known variable star
13:21:49.46 +55:12:48.3 -- not a known variable star
13:21:55.08 +49:00:50.0 -- not a known variable star
13:22:25.92 +52:52:38.0 -- not a known variable star
13:22:37.33 +53:41:48.0 -- not a known variable star
13:22:46.96 +49:26:33.2 -- not a known variable star
13:23:08.24 +48:53:15.0 -- not a known variable star
13:23:14.46 +54:05:55.4 -- not a known variable star
13:24:26.24 +55:08:38.4 -- not a known variable star
13:24:29.31 +54:14:53.6 -- not a known variable star
13:24:48.58 +55:47:30.1 -- not a known variable star
13:25:44.53 +53:56:26.7 -- not a known variable star
13:26:11.86 +54:29:22.2 -- not a known variable star
13:26:19.86 +54:59:31.7 -- not a known variable star
13:29:18.84 +54:46:28.5 -- not a known variable star
13:36:50.74 +56:24:10.7 -- not a known variable star
13:49:19.07 +53:57:26.8 -- not a known variable star
14:25:00.92 +55:32:49.9 -- not a known variable star
14:50:43.25 +51:16:27.1 -- not a known variable star
14:51:54.75 +51:47:00.2 -- a known variable star
14:52:19.92 +56:35:58.8 -- not a known variable star
14:54:05.90 +54:01:27.5 -- not a known variable star
14:57:06.97 +54:46:29.1 -- not a known variable star
Found 67 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
75 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 75 (excluding asteroids and hot pixels, 67 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)2461258.72434925 -observatory V36
07:45:39.47 +20:23:15.2 Mercury (-0.3mag)
11:55:42.14 -00:04:08.8 Venus (-4.3mag)
05:43:27.24 +23:32:40.2 Mars (1.3mag)
08:41:08.39 +18:47:57.2 Jupiter (-1.8mag)
00:56:32.95 +03:16:46.9 Saturn (0.6mag)
04:11:29.75 +20:56:20.7 Uranus (5.8mag)
00:16:12.78 +00:13:58.7 Neptune (7.7mag)
20:28:19.97 -23:29:24.4 Pluto (14.4mag)
02:47:17.00 +20:37:26.4 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 00:26 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461258.72434925:
08:41:15.25 +18:47:28.0 Io (6.0mag)
08:41:05.05 +18:48:12.0 Europa (6.3mag)
08:41:04.99 +18:48:15.7 Ganymede (5.6mag)
08:40:54.69 +18:48:58.8 Callisto (6.7mag)
08:38:44.27 +18:46:07.3 Himalia (15.7mag)
08:41:06.56 +18:48:05.8 Thebe (16.6mag)
08:38:14.91 +18:45:02.5 Elara (17.7mag)
08:45:14.30 +18:28:21.8 Pasiphae (17.9mag)
08:44:27.19 +18:57:47.7 Carme (19.0mag)
00:56:30.69 +03:17:13.8 Titan (8.4mag)
00:56:27.21 +03:16:50.5 Rhea (9.7mag)
00:56:36.60 +03:15:09.1 Iapetus (11.1mag)
00:56:19.54 +03:17:01.2 Hyperion (14.4mag)
00:55:57.98 +03:10:13.5 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 00:27 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.72434925:
18:55:35.34 -24:03:24.7 JWST
17:13:59.93 +41:40:55.4 Chandra
09:27:35.14 -53:25:10.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 00:26 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.72434925 -observatory V36
03:11:23.56 +17:12:28.0 17.7mag P/1996 R2 (Lagerkvist)
18:02:24.48 -34:38:23.9 14.0mag P/2010 H2 (Vales)
06:51:55.20 -68:49:39.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:17.10 +32:57:05.5 17.7mag C/2017 K2 (PANSTARRS)
03:37:43.73 +36:44:00.0 16.7mag P/2021 N1 (ZTF)
22:40:16.58 +31:33:55.5 17.3mag C/2022 E2 (ATLAS)
06:41:29.06 +26:34:31.3 16.8mag C/2022 N2 (PANSTARRS)
10:19:43.13 +28:33:34.6 17.0mag C/2022 QE78 (ATLAS)
09:27:31.19 +05:17:43.4 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.21 -12:12:28.9 17.9mag P/2023 B1 (PANSTARRS)
21:13:24.84 +66:13:54.0 17.9mag C/2023 H5 (Lemmon)
15:49:54.14 -12:44:57.3 14.3mag C/2023 R1 (PANSTARRS)
08:05:50.36 +31:15:21.1 15.2mag C/2024 E1 (Wierzchos)
15:07:17.74 +15:36:58.7 17.7mag C/2024 G6 (ATLAS)
19:05:40.21 +42:57:42.8 13.7mag C/2024 J3 (ATLAS)
21:13:39.90 +49:04:43.3 17.6mag C/2024 R4 (PANSTARRS)
05:13:31.47 -12:59:38.2 15.5mag C/2024 T5 (ATLAS)
06:54:54.99 +24:30:27.6 17.9mag C/2025 J1 (Borisov)
07:29:56.97 -15:52:01.8 17.7mag C/2025 R3 (PANSTARRS)
10:30:07.67 +21:01:51.8 17.3mag C/2025 V2 (Rankin)
12:56:56.48 +02:28:55.1 17.0mag C/2025 Y1 (ATLAS)
16:03:41.99 +78:01:06.2 16.8mag C/2026 A2 (Bok)
03:06:43.06 +46:08:43.0 17.1mag C/2026 B2 (Sun-Gao)
11:45:08.89 +08:19:57.7 17.3mag A/2026 E1
21:56:07.05 -26:27:24.7 6.9mag 10P/Tempel
11:27:46.06 -03:16:35.5 16.2mag 29P/Schwassmann-Wachmann
04:36:45.49 +32:15:43.8 18.0mag 47P/Ashbrook-Jackson
11:03:36.60 +05:17:46.9 17.2mag 63P/Wild
00:54:17.92 -05:22:42.8 15.4mag 65P/Gunn
05:31:00.18 +20:43:46.4 13.7mag 78P/Gehrels
20:39:47.47 -23:17:32.1 17.8mag 84P/Giclas
02:58:43.53 +13:32:23.0 16.7mag 88P/Howell
07:50:45.86 +27:55:42.1 16.1mag 93P/Lovas
04:00:44.02 +16:05:48.4 17.6mag 112P/Urata-Niijima
05:49:52.21 +30:30:52.7 16.3mag 114P/Wiseman-Skiff
09:13:44.91 +26:59:09.4 15.0mag 123P/West-Hartley
11:39:44.10 -09:29:54.8 17.1mag 124P/Mrkos
05:33:35.88 +21:11:10.5 16.1mag 128P/Shoemaker-Holt
06:25:05.10 +18:59:46.0 17.9mag 131P/Mueller
00:03:41.84 +03:25:21.6 17.6mag 139P/Vaisala-Oterma
03:21:34.08 -19:44:54.1 14.0mag 161P/Hartley-IRAS
07:09:14.42 +37:41:23.4 15.8mag 162P/SidingSpring
15:49:55.53 +39:29:36.3 12.3mag 169P/NEAT
02:39:18.44 +09:28:31.8 17.6mag 220P/McNaught
16:40:35.33 -09:56:40.2 17.6mag 235P/LINEAR
20:23:43.96 -52:50:56.0 17.8mag 259P/Garradd
03:16:17.16 +24:19:11.5 15.4mag 260P/McNaught
06:59:20.26 +37:45:17.0 17.3mag 295P/LINEAR
15:09:50.98 +03:21:31.9 17.7mag 391P/Kowalski
08:59:03.69 +18:28:26.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 00:26 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 00:26 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 00:26 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 00:26 tns_transients_list.txt
