This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd
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 06 15.1657 2461206.6657 12.39 14:38:36.92 +33:03:40.9
53.84926 66.14297 galactic Boo Second-epoch detections are separated by 0.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:36.92 +33:03:40.9 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:36.92 +33:03:40.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:36.92 +33:03:40.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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,2461206.6657,12.39,0.05,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 20260615.1657 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.44 14:45:41.56 +33:56:14.9
55.46853 64.56537 galactic Boo Second-epoch detections are separated by 0.6" and 4.0 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 | Large-amplitude variable Gaia DR2 1292842128839202432 | 14:45:41.56 +33:56:14.9 (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) SpType: G8 (LAMOST DR5) J-Ks=0.478+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:41.56 +33:56:14.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:41.56 +33:56:14.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 1292842128839202432,2461206.6657,12.44,0.05,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
Large-amplitude variable Gaia DR2 1292842128839202432 20260615.1657 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 06 15.1657 2461206.6657 12.13 14:38:58.30 +32:58:24.2
53.61077 66.07979 galactic Boo Second-epoch detections are separated by 1.6" and 4.2 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 | 14:38:58.30 +32:58:24.2 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.749+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:58.30 +32:58:24.2: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:58.30 +32:58:24.2: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.13,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.46 14:40:08.44 +34:03:57.7
56.17424 65.68452 galactic Boo Second-epoch detections are separated by 1.3" and 4.1 pix
The object was found in VSX 0" Gaia DR3 1287639033658600320
Type: ROT
# Max. Min./Amp. JD0 Period
13.120 G 13.150 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:08.44 +34:03:57.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:08.44 +34:03:57.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 1287639033658600320,2461206.6657,12.46,0.05,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
Gaia DR3 1287639033658600320 20260615.1657 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 06 15.1657 2461206.6657 12.49 14:47:32.83 +35:00:24.8
57.77304 64.02603 galactic Boo Second-epoch detections are separated by 1.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:32.83 +35:00:24.8 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:32.83 +35:00:24.8: 13.44 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:32.83 +35:00:24.8: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461206.6657,12.49,0.05,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 20260615.1657 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.38 14:38:41.93 +32:44:48.0
53.07131 66.16347 galactic Boo Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:41.93 +32:44:48.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:41.93 +32:44:48.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:41.93 +32:44:48.0: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461206.6657,12.38,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.61 14:37:47.77 +34:53:56.4
58.38933 66.00995 galactic Boo Second-epoch detections are separated by 2.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:37:47.77 +34:53:56.4 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:37:47.77 +34:53:56.4: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:47.77 +34:53:56.4: 13.41 +/- 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!
Don'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,2461206.6657,12.61,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 12.58 14:47:05.29 +33:40:44.3
54.78821 64.31103 galactic Boo Second-epoch detections are separated by 2.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:05.29 +33:40:44.3 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.342+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:05.29 +33:40:44.3: 13.67 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:05.29 +33:40:44.3: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
target,2461206.6657,12.58,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 12.73 14:41:51.32 +34:17:46.9
56.58475 65.29746 galactic Boo Second-epoch detections are separated by 0.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:51.32 +34:17:46.9 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.276+/-0.033 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:51.32 +34:17:46.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:51.32 +34:17:46.9: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.73,0.05,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 20260615.1657 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.88 14:40:22.54 +33:36:18.1
55.04910 65.70569 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 pix
The object was found in VSX 1" Gaia DR3 1287608178613517312
Type: ROT
# Max. Min./Amp. JD0 Period
13.690 G 13.730 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:22.54 +33:36:18.1: 14.00 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:22.54 +33:36:18.1: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
Gaia DR3 1287608178613517312,2461206.6657,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1287608178613517312 20260615.1657 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.62 14:46:18.36 +34:32:53.4
56.82728 64.35133 galactic Boo Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:46:18.36 +34:32:53.4 (user input) | T | P | (position from user input) J-Ks=0.826+/-0.028 (M)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.36 +34:32:53.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.36 +34:32:53.4: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461206.6657,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.48 14:38:02.79 +34:17:52.0
56.91133 66.07253 galactic Boo Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:02.79 +34:17:52.0 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:02.79 +34:17:52.0: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:02.79 +34:17:52.0: 13.41 +/- 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,2461206.6657,12.48,0.05,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 20260615.1657 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.49 14:46:18.89 +34:17:09.6
56.22744 64.38892 galactic Boo Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J221.5739+34.2949 | 14:46:18.89 +34:17:09.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.356+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.89 +34:17:09.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.89 +34:17:09.6: 13.52 +/- 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
ATO J221.5739+34.2949,2461206.6657,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J221.5739+34.2949 20260615.1657 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.64 14:31:07.69 +33:20:04.1
55.11918 67.65285 galactic Boo Second-epoch detections are separated by 0.9" and 4.2 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 | 14:31:07.69 +33:20:04.1 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.036 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:07.69 +33:20:04.1: 13.50 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:07.69 +33:20:04.1: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 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,2461206.6657,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.55 14:38:09.09 +32:47:43.7
53.22462 66.27208 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 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 1286715203375684480 | 14:38:09.11 +32:47:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.306+/-0.031 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:09.09 +32:47:43.7: 12.53 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:09.09 +32:47:43.7: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 1286715203375684480,2461206.6657,11.55,0.05,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
Gaia DR3 1286715203375684480 20260615.1657 11.55CV 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 06 15.1657 2461206.6657 11.63 14:39:23.91 +33:26:36.0
54.72791 65.92999 galactic Boo Second-epoch detections are separated by 1.1" and 4.2 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 | Gaia DR3 1287512108785770368 | 14:39:23.91 +33:26:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.241+/-0.033 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:23.91 +33:26:36.0: 12.53 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:23.91 +33:26:36.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1287512108785770368,2461206.6657,11.63,0.05,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 1287512108785770368 20260615.1657 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 06 15.1657 2461206.6657 11.51 14:40:51.66 +32:44:59.7
52.95580 65.71128 galactic Boo Second-epoch detections are separated by 0.4" and 4.0 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 J220.2166+32.7467 | 14:40:51.66 +32:44:59.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.344+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:51.66 +32:44:59.7: 12.55 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:51.66 +32:44:59.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J220.2166+32.7467,2461206.6657,11.51,0.05,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 J220.2166+32.7467 20260615.1657 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 13.01 14:39:49.42 +32:55:42.7
53.44867 65.90772 galactic Boo Second-epoch detections are separated by 5.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:49.42 +32:55:42.7 (user input) | T | P | (position from user input) J-Ks=0.792+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:49.42 +32:55:42.7: 14.24 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:49.42 +32:55:42.7: 14.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.06
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,2461206.6657,13.01,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.49 14:42:58.35 +34:28:17.5
56.90674 65.04148 galactic Boo Second-epoch detections are separated by 0.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:58.35 +34:28:17.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.389+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:58.35 +34:28:17.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:58.35 +34:28:17.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 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,2461206.6657,12.49,0.05,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 20260615.1657 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.65 14:42:35.46 +33:31:52.6
54.72155 65.25857 galactic Boo Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1286845804739350912 | 14:42:35.47 +33:31:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.513+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:35.46 +33:31:52.6: 12.67 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:35.46 +33:31:52.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 1286845804739350912,2461206.6657,11.65,0.05,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 1286845804739350912 20260615.1657 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.63 14:39:06.28 +33:18:57.0
54.43836 66.00819 galactic Boo Second-epoch detections are separated by 0.8" and 3.9 pix
The object was found in VSX 2" Gaia DR3 1287505133758803712
Type: ROT
# Max. Min./Amp. JD0 Period
13.320 G 13.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:06.28 +33:18:57.0: 13.71 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:06.28 +33:18:57.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 1287505133758803712,2461206.6657,12.63,0.05,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 1287505133758803712 20260615.1657 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.66 14:40:19.70 +34:44:54.8
57.78611 65.52890 galactic Boo Second-epoch detections are separated by 1.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:19.70 +34:44:54.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.474+/-0.037 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:19.70 +34:44:54.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:19.70 +34:44:54.8: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461206.6657,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.80 14:41:36.27 +34:01:24.2
55.95812 65.39167 galactic Boo Second-epoch detections are separated by 0.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:36.27 +34:01:24.2 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.372+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:36.27 +34:01:24.2: 12.71 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:36.27 +34:01:24.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,11.80,0.05,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 20260615.1657 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.56 14:44:36.44 +33:27:30.7
54.42459 64.85074 galactic Boo Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:36.44 +33:27:30.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.396+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:36.44 +33:27:30.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:36.44 +33:27:30.7: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
target,2461206.6657,12.56,0.05,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 20260615.1657 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.74 14:40:05.44 +33:03:53.4
53.76333 65.83582 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:05.44 +33:03:53.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.313+/-0.033 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:05.44 +33:03:53.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:05.44 +33:03:53.4: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 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
target,2461206.6657,12.74,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.76 14:44:06.07 +34:19:01.8
56.45934 64.83623 galactic Boo Second-epoch detections are separated by 1.1" and 3.9 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 1292909851884117888 | 14:44:06.10 +34:19:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.461+/-0.026 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:06.07 +34:19:01.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:06.07 +34:19:01.8: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1292909851884117888,2461206.6657,11.76,0.05,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
Gaia DR3 1292909851884117888 20260615.1657 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 06 15.1657 2461206.6657 12.71 14:43:08.60 +34:13:57.0
56.33416 65.04483 galactic Boo Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:08.60 +34:13:57.0 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.637+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:08.60 +34:13:57.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:08.60 +34:13:57.0: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 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
target,2461206.6657,12.71,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 12.65 14:43:43.22 +33:04:52.1
53.58964 65.07869 galactic Boo Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J220.9303+33.0814 | 14:43:43.22 +33:04:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.501+/-0.041 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:43.22 +33:04:52.1: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:43.22 +33:04:52.1: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J220.9303+33.0814,2461206.6657,12.65,0.05,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 J220.9303+33.0814 20260615.1657 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.04 14:38:47.35 +33:50:08.0
55.72623 65.99765 galactic Boo Second-epoch detections are separated by 0.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:47.35 +33:50:08.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.282+/-0.031 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:47.35 +33:50:08.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:47.35 +33:50:08.0: 12.98 +/- 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!
Don'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,2461206.6657,12.04,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.97 14:39:29.80 +33:13:49.2
54.20356 65.93831 galactic Boo Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:29.80 +33:13:49.2 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:29.80 +33:13:49.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:29.80 +33:13:49.2: 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!
Don'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,2461206.6657,11.97,0.05,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 20260615.1657 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.57 14:43:46.91 +33:42:17.2
55.05249 64.98990 galactic Boo Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:46.91 +33:42:17.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.476+/-0.032 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:46.91 +33:42:17.2: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:46.91 +33:42:17.2: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461206.6657,12.57,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.18 14:31:43.91 +32:58:42.6
54.14398 67.58361 galactic Boo Second-epoch detections are separated by 0.4" and 3.9 pix
The object was found in VSX 1" Gaia DR3 1287330964245099520
Type: ROT
# Max. Min./Amp. JD0 Period
12.870 G 12.900 G 4.965050000000 G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:43.91 +32:58:42.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:43.91 +32:58:42.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1287330964245099520,2461206.6657,12.18,0.05,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
Gaia DR3 1287330964245099520 20260615.1657 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 06 15.1657 2461206.6657 12.04 14:45:28.10 +33:49:23.4
55.21897 64.62678 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:45:28.10 +33:49:23.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.677+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:28.10 +33:49:23.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:28.10 +33:49:23.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.04,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.04 14:46:41.03 +33:57:01.9
55.43475 64.35991 galactic Boo Second-epoch detections are separated by 0.8" and 3.8 pix
The object was found in VSX 1" Gaia DR3 1292830858845055488
Type: ROT
# Max. Min./Amp. JD0 Period
12.790 G 12.840 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:41.03 +33:57:01.9: 13.03 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:41.03 +33:57:01.9: 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
Gaia DR3 1292830858845055488,2461206.6657,12.04,0.05,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
Gaia DR3 1292830858845055488 20260615.1657 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 06 15.1657 2461206.6657 12.04 14:38:37.97 +33:10:01.8
54.10743 66.12572 galactic Boo Second-epoch detections are separated by 0.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:37.97 +33:10:01.8 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:37.97 +33:10:01.8: 13.02 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:37.97 +33:10:01.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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,2461206.6657,12.04,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.09 14:42:12.27 +34:00:50.5
55.89081 65.27019 galactic Boo Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:12.27 +34:00:50.5 (user input) | T | P | (position from user input) J-Ks=0.257+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:12.27 +34:00:50.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:12.27 +34:00:50.5: 13.05 +/- 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,2461206.6657,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 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 06 15.1657 2461206.6657 12.73 14:44:37.70 +33:13:08.2
53.86326 64.87444 galactic Boo Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:37.70 +33:13:08.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.471+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:37.70 +33:13:08.2: 13.94 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:37.70 +33:13:08.2: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
target,2461206.6657,12.73,0.05,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 20260615.1657 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.70 14:38:38.21 +34:56:25.9
58.40494 65.83281 galactic Boo Second-epoch detections are separated by 4.6" and 4.5 pix
The object was found in VSX 3" Gaia DR3 1287944560451650816
Type: ROT
# Max. Min./Amp. JD0 Period
13.450 G 13.490 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:38.21 +34:56:25.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:38.21 +34:56:25.9: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 1287944560451650816,2461206.6657,12.70,0.05,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 1287944560451650816 20260615.1657 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.69 14:44:38.13 +34:39:34.9
57.21090 64.67281 galactic Boo Second-epoch detections are separated by 1.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:38.13 +34:39:34.9 (user input) | T | P | (position from user input) SpType: A6IV (LAMOST DR5) J-Ks=0.136+/-0.037 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:38.13 +34:39:34.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:38.13 +34:39:34.9: 13.57 +/- 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
target,2461206.6657,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.78 14:40:21.50 +32:42:29.1
52.88209 65.82087 galactic Boo Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:21.50 +32:42:29.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.468+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:21.50 +32:42:29.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:21.50 +32:42:29.1: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
target,2461206.6657,12.78,0.05,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 20260615.1657 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.54 14:40:14.26 +33:07:35.3
53.90343 65.79770 galactic Boo Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:14.26 +33:07:35.3 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.610+/-0.031 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:14.26 +33:07:35.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:14.26 +33:07:35.3: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461206.6657,12.54,0.05,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 20260615.1657 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.93 14:43:54.02 +32:49:21.7
52.97039 65.06838 galactic Boo Second-epoch detections are separated by 0.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:54.02 +32:49:21.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.335+/-0.036 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:54.02 +32:49:21.7: 14.12 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:54.02 +32:49:21.7: 14.21 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
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,2461206.6657,12.93,0.05,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 20260615.1657 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.51 14:38:56.04 +32:46:01.1
53.10723 66.11203 galactic Boo Second-epoch detections are separated by 0.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:56.04 +32:46:01.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.409+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:56.04 +32:46:01.1: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:56.04 +32:46:01.1: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461206.6657,12.51,0.05,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 20260615.1657 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.71 14:45:40.12 +34:06:19.0
55.85696 64.54708 galactic Boo Second-epoch detections are separated by 1.8" and 4.2 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 | 14:45:40.12 +34:06:19.0 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:40.12 +34:06:19.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:40.12 +34:06:19.0: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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
target,2461206.6657,12.71,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 11.72 14:40:00.82 +32:59:49.8
53.60392 65.86001 galactic Boo Second-epoch detections are separated by 0.7" and 4.0 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 J220.0032+32.9971 | 14:40:00.82 +32:59:49.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:00.82 +32:59:49.8: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:00.82 +32:59:49.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J220.0032+32.9971,2461206.6657,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J220.0032+32.9971 20260615.1657 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.62 14:45:19.07 +33:50:39.5
55.27756 64.65496 galactic Boo Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:45:19.07 +33:50:39.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.518+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:19.07 +33:50:39.5: 13.77 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:19.07 +33:50:39.5: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
target,2461206.6657,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.90 14:44:25.67 +33:04:03.3
53.51947 64.93284 galactic Boo Second-epoch detections are separated by 1.9" and 4.2 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 | 14:44:25.67 +33:04:03.3 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.034 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:25.67 +33:04:03.3: 14.24 +/- 0.08 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:25.67 +33:04:03.3: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
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,2461206.6657,12.90,0.05,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 20260615.1657 12.90CV 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 06 15.1657 2461206.6657 11.28 14:45:20.67 +33:35:20.7
54.68432 64.68225 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 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 1286814258201490560 | 14:45:20.72 +33:35:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:20.67 +33:35:20.7: 12.30 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:20.67 +33:35:20.7: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 1286814258201490560,2461206.6657,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1286814258201490560 20260615.1657 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.48 14:42:27.30 +33:34:33.7
54.83653 65.28074 galactic Boo Second-epoch detections are separated by 1.4" and 4.2 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 | 14:42:27.30 +33:34:33.7 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.041 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:27.30 +33:34:33.7: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:27.30 +33:34:33.7: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 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,2461206.6657,12.48,0.05,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 20260615.1657 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.88 14:47:21.14 +35:19:44.3
58.51290 64.00969 galactic Boo Second-epoch detections are separated by 2.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:21.14 +35:19:44.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.480+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:21.14 +35:19:44.3: 13.88 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:21.14 +35:19:44.3: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 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
target,2461206.6657,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.71 14:41:14.37 +34:10:10.8
56.33380 65.44346 galactic Boo Second-epoch detections are separated by 2.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:14.37 +34:10:10.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:14.37 +34:10:10.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:14.37 +34:10:10.8: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
target,2461206.6657,12.71,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 12.92 14:40:51.93 +33:37:42.1
55.07025 65.60144 galactic Boo Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:51.93 +33:37:42.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.513+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:51.93 +33:37:42.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:51.93 +33:37:42.1: 14.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
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,2461206.6657,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.90 14:46:18.85 +33:35:24.2
54.62906 64.48171 galactic Boo Second-epoch detections are separated by 0.1" and 3.9 pix
The object was found in VSX 1" Gaia DR3 1292627620993345792
Type: ROT
# Max. Min./Amp. JD0 Period
12.700 G 12.730 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.85 +33:35:24.2: 12.99 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.85 +33:35:24.2: 13.06 +/- 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
Gaia DR3 1292627620993345792,2461206.6657,11.90,0.05,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
Gaia DR3 1292627620993345792 20260615.1657 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 06 15.1657 2461206.6657 12.74 14:30:14.73 +33:08:23.9
54.69118 67.86652 galactic Boo Second-epoch detections are separated by 0.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:30:14.73 +33:08:23.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.402+/-0.036 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:14.73 +33:08:23.9: 13.54 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:14.73 +33:08:23.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461206.6657,12.74,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.82 14:39:05.73 +32:54:06.9
53.42812 66.06261 galactic Boo Second-epoch detections are separated by 2.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:05.73 +32:54:06.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.412+/-0.035 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:05.73 +32:54:06.9: 13.87 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:05.73 +32:54:06.9: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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
target,2461206.6657,12.82,0.05,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 20260615.1657 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.79 14:38:57.23 +33:54:23.5
55.88522 65.95275 galactic Boo Second-epoch detections are separated by 2.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:57.23 +33:54:23.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:57.23 +33:54:23.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:57.23 +33:54:23.5: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 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
target,2461206.6657,12.79,0.05,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 20260615.1657 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.54 14:40:31.57 +33:39:04.5
55.14942 65.66811 galactic Boo Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:31.57 +33:39:04.5 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:31.57 +33:39:04.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:31.57 +33:39:04.5: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461206.6657,12.54,0.05,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 20260615.1657 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.69 14:44:31.97 +35:36:12.3
59.38310 64.52169 galactic Boo Second-epoch detections are separated by 0.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:31.97 +35:36:12.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.362+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:31.97 +35:36:12.3: 13.51 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:31.97 +35:36:12.3: 13.69 +/- 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
target,2461206.6657,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.57 14:47:03.20 +33:55:57.0
55.37026 64.28630 galactic Boo Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:03.20 +33:55:57.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.423+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:03.20 +33:55:57.0: 13.74 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:03.20 +33:55:57.0: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
target,2461206.6657,12.57,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.98 14:38:26.80 +32:48:05.0
53.22112 66.20979 galactic Boo Second-epoch detections are separated by 1.0" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:38:26.80 +32:48:05.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.549+/-0.032 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:26.80 +32:48:05.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:26.80 +32:48:05.0: 13.13 +/- 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,2461206.6657,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 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 06 15.1657 2461206.6657 11.93 14:40:20.22 +33:38:09.5
55.12634 65.70926 galactic Boo Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:20.22 +33:38:09.5 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:20.22 +33:38:09.5: 12.96 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:20.22 +33:38:09.5: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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,2461206.6657,11.93,0.05,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 20260615.1657 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.56 14:40:12.83 +32:50:49.8
53.22786 65.83573 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:12.83 +32:50:49.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.452+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:12.83 +32:50:49.8: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:12.83 +32:50:49.8: 13.84 +/- 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
target,2461206.6657,12.56,0.05,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 20260615.1657 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.94 14:44:00.28 +33:31:51.8
54.63101 64.96644 galactic Boo Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:00.28 +33:31:51.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.388+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:00.28 +33:31:51.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:00.28 +33:31:51.8: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461206.6657,11.94,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 10.44 14:41:26.95 +32:54:47.6
53.31658 65.57059 galactic Boo Second-epoch detections are separated by 0.6" and 4.0 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 1286688230981104640 | 14:41:27.00 +32:54:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.380+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:26.95 +32:54:47.6: 11.40 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:26.95 +32:54:47.6: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
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 1286688230981104640,2461206.6657,10.44,0.05,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
Gaia DR3 1286688230981104640 20260615.1657 10.44CV 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 06 15.1657 2461206.6657 12.31 14:45:54.62 +34:16:35.6
56.23408 64.47296 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:45:54.62 +34:16:35.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.402+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:54.62 +34:16:35.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:54.62 +34:16:35.6: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461206.6657,12.31,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.57 14:42:19.70 +33:49:51.2
55.44875 65.27164 galactic Boo Second-epoch detections are separated by 0.8" and 4.0 pix
The object was found in VSX 2" Gaia DR3 1286888032857821824
Type: VAR
# Max. Min./Amp. JD0 Period
13.420 G 13.480 G 0.031075000000 A
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:19.70 +33:49:51.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:19.70 +33:49:51.2: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 1286888032857821824,2461206.6657,12.57,0.05,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
Gaia DR3 1286888032857821824 20260615.1657 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 06 15.1657 2461206.6657 12.47 14:42:09.13 +34:19:08.3
56.61436 65.23331 galactic Boo Second-epoch detections are separated by 2.1" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:09.13 +34:19:08.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.389+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:09.13 +34:19:08.3: 13.32 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:09.13 +34:19:08.3: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.18 14:45:41.81 +33:16:28.0
53.93395 64.64623 galactic Boo Second-epoch detections are separated by 0.9" and 3.9 pix
The object was found in VSX13" Gaia DR3 1286617862236631296
Type: ROT
# Max. Min./Amp. JD0 Period
12.480 G 12.510 G M
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:41.81 +33:16:28.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:41.81 +33:16:28.0: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 1286617862236631296,2461206.6657,12.18,0.05,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
Gaia DR3 1286617862236631296 20260615.1657 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 06 15.1657 2461206.6657 12.42 14:30:15.10 +33:13:53.4
54.93028 67.85044 galactic Boo Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:30:15.10 +33:13:53.4 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.035 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:15.10 +33:13:53.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:15.10 +33:13:53.4: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.42,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.57 14:41:13.71 +32:52:10.4
53.22400 65.62148 galactic Boo Second-epoch detections are separated by 0.6" and 3.9 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 1286682080588716160 | 14:41:13.69 +32:52:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.242+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:13.71 +32:52:10.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:13.71 +32:52:10.4: 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 1286682080588716160,2461206.6657,11.57,0.05,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
Gaia DR3 1286682080588716160 20260615.1657 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.78 14:43:53.18 +33:17:19.5
54.06920 65.02050 galactic Boo Second-epoch detections are separated by 2.1" and 4.2 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 | 14:43:53.18 +33:17:19.5 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:53.18 +33:17:19.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:53.18 +33:17:19.5: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
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,2461206.6657,12.78,0.05,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 20260615.1657 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 11.72 14:38:40.15 +33:25:18.8
54.72792 66.08366 galactic Boo Second-epoch detections are separated by 0.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1287509737963754368 | 14:38:40.16 +33:25:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.279+/-0.032 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:40.15 +33:25:18.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:40.15 +33:25:18.8: 12.68 +/- 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 1287509737963754368,2461206.6657,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1287509737963754368 20260615.1657 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.49 14:45:59.09 +33:26:07.0
54.29063 64.56820 galactic Boo Second-epoch detections are separated by 1.0" and 3.8 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 1286621607447543808 | 14:45:59.06 +33:26:07.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.337+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:59.09 +33:26:07.0: 12.56 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:59.09 +33:26:07.0: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 1286621607447543808,2461206.6657,11.49,0.05,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 1286621607447543808 20260615.1657 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.55 14:41:41.28 +33:16:00.6
54.14993 65.47924 galactic Boo Second-epoch detections are separated by 0.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1286834947061973248 | 14:41:41.29 +33:16:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.416+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:41.28 +33:16:00.6: 12.56 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:41.28 +33:16:00.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 1286834947061973248,2461206.6657,11.55,0.05,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
Gaia DR3 1286834947061973248 20260615.1657 11.55CV 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 06 15.1657 2461206.6657 12.91 14:46:47.00 +33:23:30.3
54.14611 64.40762 galactic Boo Second-epoch detections are separated by 1.6" and 4.0 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 J221.6948+33.3959 | 14:46:47.00 +33:23:30.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.390+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:47.00 +33:23:30.3: 14.12 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:47.00 +33:23:30.3: 14.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J221.6948+33.3959,2461206.6657,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J221.6948+33.3959 20260615.1657 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.95 14:42:55.98 +32:56:36.8
53.30691 65.25778 galactic Boo Second-epoch detections are separated by 0.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:55.98 +32:56:36.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.579+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:55.98 +32:56:36.8: 14.21 +/- 0.08 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:55.98 +32:56:36.8: 14.16 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
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,2461206.6657,12.95,0.05,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 20260615.1657 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.22 14:43:39.43 +32:50:36.8
53.03193 65.11709 galactic Boo Second-epoch detections are separated by 0.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:39.43 +32:50:36.8 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.525+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:39.43 +32:50:36.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:39.43 +32:50:36.8: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461206.6657,12.22,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.44 14:29:22.45 +32:57:09.8
54.27485 68.07633 galactic Boo Second-epoch detections are separated by 2.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:29:22.45 +32:57:09.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.574+/-0.034 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:22.45 +32:57:09.8: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:22.45 +32:57:09.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.44,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.69 14:48:21.86 +35:32:14.3
58.89415 63.76939 galactic Boo Second-epoch detections are separated by 0.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:48:21.86 +35:32:14.3 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.394+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:48:21.86 +35:32:14.3: 13.71 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:48:21.86 +35:32:14.3: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461206.6657,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.96 14:40:19.53 +33:50:46.4
55.63248 65.68077 galactic Boo Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:19.53 +33:50:46.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.554+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:19.53 +33:50:46.4: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:19.53 +33:50:46.4: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461206.6657,11.96,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.46 14:42:30.21 +33:41:19.6
55.10029 65.25550 galactic Boo Second-epoch detections are separated by 1.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:30.21 +33:41:19.6 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:30.21 +33:41:19.6: 13.49 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:30.21 +33:41:19.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461206.6657,12.46,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.38 14:46:06.19 +34:11:31.7
56.02697 64.44575 galactic Boo Second-epoch detections are separated by 2.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:46:06.19 +34:11:31.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:06.19 +34:11:31.7: 13.48 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:06.19 +34:11:31.7: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.38,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.69 14:47:24.88 +34:26:50.8
56.51866 64.14075 galactic Boo Second-epoch detections are separated by 0.6" and 3.9 pix
The object was found in VSX 1" Gaia DR3 1292882879489008256
Type: ROT
# Max. Min./Amp. JD0 Period
13.320 G 13.400 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:24.88 +34:26:50.8: 13.70 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:24.88 +34:26:50.8: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
Gaia DR3 1292882879489008256,2461206.6657,12.69,0.05,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 1292882879489008256 20260615.1657 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.49 14:39:41.55 +33:18:44.0
54.38928 65.88697 galactic Boo Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:41.55 +33:18:44.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.375+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:41.55 +33:18:44.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:41.55 +33:18:44.0: 13.58 +/- 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,2461206.6657,12.49,0.05,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 20260615.1657 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.39 14:47:19.41 +34:36:45.4
56.89947 64.13446 galactic Boo Second-epoch detections are separated by 2.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:19.41 +34:36:45.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.279+/-0.031 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:19.41 +34:36:45.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:19.41 +34:36:45.4: 13.51 +/- 0.05 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!
Don'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,2461206.6657,12.39,0.05,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 20260615.1657 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.22 14:40:00.41 +32:52:38.2
53.31311 65.87549 galactic Boo Second-epoch detections are separated by 1.8" and 4.3 pix
The object was found in VSX 1" Gaia DR3 1286729119069700096
Type: ROT
# Max. Min./Amp. JD0 Period
13.250 G 13.280 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:00.41 +32:52:38.2: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:00.41 +32:52:38.2: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 1286729119069700096,2461206.6657,12.22,0.05,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
Gaia DR3 1286729119069700096 20260615.1657 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 06 15.1657 2461206.6657 12.46 14:30:35.86 +32:51:27.7
53.92127 67.83681 galactic Boo Second-epoch detections are separated by 0.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:30:35.86 +32:51:27.7 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.034 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:35.86 +32:51:27.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:35.86 +32:51:27.7: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461206.6657,12.46,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.81 14:43:36.97 +33:24:51.0
54.38035 65.06140 galactic Boo Second-epoch detections are separated by 0.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:36.97 +33:24:51.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.401+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:36.97 +33:24:51.0: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:36.97 +33:24:51.0: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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
target,2461206.6657,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.84 14:40:13.55 +32:59:16.1
53.56828 65.81695 galactic Boo Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:13.55 +32:59:16.1 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.562+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:13.55 +32:59:16.1: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:13.55 +32:59:16.1: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 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
target,2461206.6657,12.84,0.05,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 20260615.1657 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.59 14:31:09.33 +33:26:17.8
55.38575 67.62993 galactic Boo Second-epoch detections are separated by 3.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:31:09.33 +33:26:17.8 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.035 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:09.33 +33:26:17.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:09.33 +33:26:17.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461206.6657,12.59,0.05,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
target 20260615.1657 12.59CV 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 06 15.1657 2461206.6657 11.11 14:46:35.14 +33:33:19.0
54.53330 64.42972 galactic Boo Second-epoch detections are separated by 0.1" and 3.9 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 1292627964590725504 | 14:46:35.16 +33:33:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.391+/-0.027 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:35.14 +33:33:19.0: 12.13 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:35.14 +33:33:19.0: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 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 1292627964590725504,2461206.6657,11.11,0.05,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
Gaia DR3 1292627964590725504 20260615.1657 11.11CV 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 06 15.1657 2461206.6657 12.87 14:40:34.03 +33:03:30.4
53.71843 65.73749 galactic Boo Second-epoch detections are separated by 1.7" and 4.2 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 | 14:40:34.03 +33:03:30.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.496+/-0.029 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:34.03 +33:03:30.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:34.03 +33:03:30.4: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
target,2461206.6657,12.87,0.05,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 20260615.1657 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.51 14:42:56.40 +33:22:17.8
54.32139 65.20671 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 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 1286794711808922240 | 14:42:56.37 +33:22:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.410+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:56.40 +33:22:17.8: 12.52 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:56.40 +33:22:17.8: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1286794711808922240,2461206.6657,11.51,0.05,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 1286794711808922240 20260615.1657 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.43 14:29:36.11 +33:15:57.6
55.08060 67.97872 galactic Boo Second-epoch detections are separated by 2.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:29:36.11 +33:15:57.6 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.585+/-0.032 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:36.11 +33:15:57.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:36.11 +33:15:57.6: 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,2461206.6657,12.43,0.05,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 20260615.1657 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.20 14:44:05.31 +33:32:48.3
54.66257 64.94713 galactic Boo Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:05.31 +33:32:48.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.292+/-0.035 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:05.31 +33:32:48.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:05.31 +33:32:48.3: 13.34 +/- 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,2461206.6657,12.20,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.20 14:42:52.59 +33:30:38.0
54.65403 65.20227 galactic Boo Second-epoch detections are separated by 0.5" and 4.0 pix
The object was found in VSX 1" Gaia DR3 1286845083184840448
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.030 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:52.59 +33:30:38.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:52.59 +33:30:38.0: 13.24 +/- 0.04 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 1286845083184840448,2461206.6657,12.20,0.05,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
Gaia DR3 1286845083184840448 20260615.1657 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 06 15.1657 2461206.6657 12.77 14:41:33.81 +34:42:17.6
57.57235 65.28724 galactic Boo Second-epoch detections are separated by 1.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:33.81 +34:42:17.6 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:33.81 +34:42:17.6: 13.66 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:33.81 +34:42:17.6: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461206.6657,12.77,0.05,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 20260615.1657 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.48 14:40:58.12 +33:16:33.8
54.21764 65.62724 galactic Boo Second-epoch detections are separated by 1.5" and 4.2 pix
The object was found in VSX 1" CSS_J144058.1+331635
Type: RRC
# Max. Min./Amp. JD0 Period
13.670 CV Y 0.190 CV 0.324321000000
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:58.12 +33:16:33.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:58.12 +33:16:33.8: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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
CSS_J144058.1+331635,2461206.6657,12.48,0.05,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
CSS_J144058.1+331635 20260615.1657 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.63 14:43:59.90 +33:25:05.9
54.36692 64.98175 galactic Boo Second-epoch detections are separated by 1.6" and 4.2 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 | 14:43:59.90 +33:25:05.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.249+/-0.035 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:59.90 +33:25:05.9: 13.67 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:59.90 +33:25:05.9: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 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
target,2461206.6657,12.63,0.05,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
target 20260615.1657 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.57 14:40:57.74 +32:44:27.4
52.92858 65.69105 galactic Boo Second-epoch detections are separated by 0.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:57.74 +32:44:27.4 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:57.74 +32:44:27.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:57.74 +32:44:27.4: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461206.6657,12.57,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.23 14:31:44.70 +32:55:38.9
54.01053 67.58835 galactic Boo Second-epoch detections are separated by 2.1" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:31:44.70 +32:55:38.9 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:44.70 +32:55:38.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:44.70 +32:55:38.9: 13.28 +/- 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!
Don'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,2461206.6657,12.23,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.27 14:39:02.52 +33:25:56.4
54.72657 66.00517 galactic Boo Second-epoch detections are separated by 2.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:39:02.52 +33:25:56.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:02.52 +33:25:56.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:02.52 +33:25:56.4: 13.29 +/- 0.04 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,2461206.6657,12.27,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.34 14:31:27.70 +32:57:35.5
54.11755 67.64240 galactic Boo Second-epoch detections are separated by 1.0" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:31:27.70 +32:57:35.5 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.031 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:27.70 +32:57:35.5: 13.17 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:27.70 +32:57:35.5: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.34,0.05,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
target 20260615.1657 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 06 15.1657 2461206.6657 11.71 14:44:30.34 +33:10:00.4
53.74787 64.90578 galactic Boo Second-epoch detections are separated by 0.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:30.34 +33:10:00.4 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.466+/-0.027 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:30.34 +33:10:00.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:30.34 +33:10:00.4: 12.83 +/- 0.03 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,2461206.6657,11.71,0.05,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
target 20260615.1657 11.71CV 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 06 15.1657 2461206.6657 12.37 14:42:58.89 +33:28:12.5
54.55180 65.18574 galactic Boo Second-epoch detections are separated by 0.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:58.89 +33:28:12.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.367+/-0.032 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:58.89 +33:28:12.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:58.89 +33:28:12.5: 13.53 +/- 0.05 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,2461206.6657,12.37,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.82 14:41:47.87 +33:25:58.9
54.53977 65.43536 galactic Boo Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:47.87 +33:25:58.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.248+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:47.87 +33:25:58.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:47.87 +33:25:58.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461206.6657,11.82,0.05,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 20260615.1657 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.54 14:41:49.41 +33:21:10.2
54.34679 65.44035 galactic Boo Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1286837008646329600 | 14:41:49.41 +33:21:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.469+/-0.032 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:49.41 +33:21:10.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:49.41 +33:21:10.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 1286837008646329600,2461206.6657,11.54,0.05,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
Gaia DR3 1286837008646329600 20260615.1657 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 06 15.1657 2461206.6657 12.11 14:45:49.30 +33:34:58.9
54.64178 64.58437 galactic Boo Second-epoch detections are separated by 0.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:45:49.30 +33:34:58.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.482+/-0.034 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:49.30 +33:34:58.9: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:49.30 +33:34:58.9: 13.31 +/- 0.04 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!
Don'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,2461206.6657,12.11,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.15 14:44:58.15 +33:59:55.7
55.65853 64.70551 galactic Boo Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:58.15 +33:59:55.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.472+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:58.15 +33:59:55.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:58.15 +33:59:55.7: 13.20 +/- 0.04 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!
Don'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,2461206.6657,12.15,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.53 14:42:32.35 +33:37:47.2
54.95823 65.25618 galactic Boo Second-epoch detections are separated by 0.9" and 4.0 pix
The object was found in VSX 0" Gaia DR3 1286850404646253312
Type: ROT
# Max. Min./Amp. JD0 Period
12.260 G 12.290 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:32.35 +33:37:47.2: 12.47 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:32.35 +33:37:47.2: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 1286850404646253312,2461206.6657,11.53,0.05,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 1286850404646253312 20260615.1657 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 10.99 14:42:06.38 +32:53:18.9
53.22091 65.43620 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 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 1286674143483740160 | 14:42:06.40 +32:53:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.306+/-0.026 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:06.38 +32:53:18.9: 11.98 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:06.38 +32:53:18.9: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 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 1286674143483740160,2461206.6657,10.99,0.05,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
Gaia DR3 1286674143483740160 20260615.1657 10.99CV 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 06 15.1657 2461206.6657 12.42 14:44:39.56 +33:44:37.7
55.08667 64.80387 galactic Boo Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:44:39.56 +33:44:37.7 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:39.56 +33:44:37.7: 13.42 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:39.56 +33:44:37.7: 13.54 +/- 0.05 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,2461206.6657,12.42,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.48 14:40:03.76 +33:30:32.3
54.83983 65.78372 galactic Boo Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:03.76 +33:30:32.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.429+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:03.76 +33:30:32.3: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:03.76 +33:30:32.3: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461206.6657,12.48,0.05,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 20260615.1657 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.52 14:29:44.53 +32:56:51.9
54.22984 68.00082 galactic Boo Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:29:44.53 +32:56:51.9 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.035 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:44.53 +32:56:51.9: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:44.53 +32:56:51.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.52,0.05,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 20260615.1657 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.43 14:37:53.69 +34:59:24.0
58.59837 65.97180 galactic Boo Second-epoch detections are separated by 0.9" and 3.8 pix
The object was found in VSX 0" LQ Boo
Type: RRAB
# Max. Min./Amp. JD0 Period
12.840 CV 13.590 CV 2451330.75000 0.564333000000
The object was not found in astcheck.
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:37:53.69 +34:59:24.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:53.69 +34:59:24.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 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
LQ Boo,2461206.6657,12.43,0.05,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
LQ Boo 20260615.1657 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.27 14:41:04.32 +32:43:16.8
52.87529 65.67020 galactic Boo Second-epoch detections are separated by 0.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:04.32 +32:43:16.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.747+/-0.026 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:04.32 +32:43:16.8: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:04.32 +32:43:16.8: 13.32 +/- 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,2461206.6657,12.27,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.07 14:41:48.74 +33:05:59.7
53.74316 65.47358 galactic Boo Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:48.74 +33:05:59.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.532+/-0.031 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:48.74 +33:05:59.7: 13.13 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:48.74 +33:05:59.7: 13.19 +/- 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!
Don'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,2461206.6657,12.07,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 12.60 14:41:03.71 +33:44:36.0
55.33137 65.54464 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:41:03.71 +33:44:36.0 (user input) | T | P | (position from user input) J-Ks=0.678+/-0.030 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:03.71 +33:44:36.0: 13.64 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:03.71 +33:44:36.0: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461206.6657,12.60,0.05,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 20260615.1657 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06 15.1657 2461206.6657 12.63 14:43:12.48 +32:45:33.9
52.85531 65.21950 galactic Boo Second-epoch detections are separated by 0.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:12.48 +32:45:33.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:12.48 +32:45:33.9: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:12.48 +32:45:33.9: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 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
target,2461206.6657,12.63,0.05,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
target 20260615.1657 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.81 14:40:28.51 +32:57:54.7
53.49852 65.76768 galactic Boo Second-epoch detections are separated by 0.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:28.51 +32:57:54.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.406+/-0.028 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:28.51 +32:57:54.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:28.51 +32:57:54.7: 12.83 +/- 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,2461206.6657,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.10 14:43:45.04 +33:35:08.0
54.77483 65.01197 galactic Boo Second-epoch detections are separated by 0.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:45.04 +33:35:08.0 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:45.04 +33:35:08.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:45.04 +33:35:08.0: 13.23 +/- 0.04 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!
Don'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,2461206.6657,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.19 14:45:38.21 +34:40:36.0
57.17152 64.46692 galactic Boo Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:45:38.21 +34:40:36.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:38.21 +34:40:36.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:38.21 +34:40:36.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.19,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.81 14:40:20.88 +33:10:15.9
54.00434 65.76924 galactic Boo Second-epoch detections are separated by 0.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:40:20.88 +33:10:15.9 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.029 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:20.88 +33:10:15.9: 12.79 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:20.88 +33:10:15.9: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461206.6657,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 11.91 14:31:04.57 +32:57:28.1
54.14381 67.72268 galactic Boo Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J217.7691+32.9579 | 14:31:04.57 +32:57:28.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.487+/-0.033 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:04.57 +32:57:28.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:04.57 +32:57:28.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J217.7691+32.9579,2461206.6657,11.91,0.05,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 J217.7691+32.9579 20260615.1657 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.66 14:43:23.54 +34:32:34.0
57.03926 64.94443 galactic Boo Second-epoch detections are separated by 3.1" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:43:23.54 +34:32:34.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.580+/-0.028 (K)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:23.54 +34:32:34.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:23.54 +34:32:34.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6657,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.62 14:46:34.79 +34:16:12.8
56.17304 64.33704 galactic Boo Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:46:34.79 +34:16:12.8 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:34.79 +34:16:12.8: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:34.79 +34:16:12.8: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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
target,2461206.6657,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.62 14:47:00.58 +34:21:27.1
56.34250 64.23657 galactic Boo Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:47:00.58 +34:21:27.1 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.030 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:00.58 +34:21:27.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:00.58 +34:21:27.1: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461206.6657,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1657 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1657 2461206.6657 12.30 14:42:25.43 +33:16:10.6
54.11111 65.32625 galactic Boo Second-epoch detections are separated by 0.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:42:25.43 +33:16:10.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.360+/-0.030 (G)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:25.43 +33:16:10.6: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:25.43 +33:16:10.6: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461206.6657,12.30,0.05,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 20260615.1657 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 06 15.1657 2461206.6657 11.28 14:45:39.19 +32:57:44.3
53.21077 64.68829 galactic Boo Second-epoch detections are separated by 0.9" and 3.8 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 1286592161151713408 | 14:45:39.20 +32:57:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.305+/-0.028 (F)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:39.19 +32:57:44.3: 12.36 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:39.19 +32:57:44.3: 12.40 +/- 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 1286592161151713408,2461206.6657,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1286592161151713408 20260615.1657 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.78582344 11.05.2026 06:51:25.145 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
First image: 2461171.78582344 11.05.2026 06:51:25.145 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Last image: 2461206.66590655 15.06.2026 03:58:44.326 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5729
Objects passed selection criteria: 5701
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 3858.75
Average stars matched: 3834.25 (99.3651 %)
Memory usage VmPeak: 112164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:30:53 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: 2461171.78582344 11.05.2026 06:51:25.145 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
First image: 2461171.78582344 11.05.2026 06:51:25.145 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Last image: 2461206.66590655 15.06.2026 03:58:44.326 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 202
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.94
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28610
Objects passed selection criteria: 28512
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: 20661.5
Average stars matched: 20305.5 (98.277 %)
Memory usage VmPeak: 133112 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:31:59 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.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: 2461206.66548191
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits exists and is non-empty
Saving wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits to local_wcs_cache/
'wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits' -> 'local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits'
wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
Saving wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits to local_wcs_cache/
'wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits'
wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits exists and is non-empty
Saving wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits to local_wcs_cache/
'wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits' -> 'local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits (1st reference image)
verification OK: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:53.396 +38:00:25.91 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:11:10.804 +38:03:28.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:10:53.396 +38:00:25.91
Second-epoch image center 14:11:10.804 +38:03:28.14
Angular distance between the image centers 0.0763 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:11:11.444 +38:03:05.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:10:53.396 +38:00:25.91
Second-epoch image center 14:11:11.444 +38:03:05.61
Angular distance between the image centers 0.0740 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 14:11:10.804 +38:03:28.14
Second-epoch second image center 14:11:11.444 +38:03:05.61
Angular distance between the image centers 0.00660 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits &> /tmp/tmp.79ffH4cBpu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.SeWRYn0Q9K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits &> /tmp/tmp.IiBSqV0BcE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits &> /tmp/tmp.uMEqmpy2dd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
The reference image (wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits) and catalog (wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat) found
'wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat' -> 'wcsmag.cat'
Read 6969 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1592 to 223.3611 deg, Dec +32.4730 to +43.2688 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 202.1592 to 223.3611 deg, Dec 32.4730 to 43.2688 deg
Loaded 4579 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): 3468 out of 3575 total matches.
Matched with Tycho-2 3575 out of 6969 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.739600
a=0.000000 b=1.000000 c=22.739600
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6969 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1592 to 223.3611 deg, Dec +32.4730 to +43.2688 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 202.1592 to 223.3611 deg, Dec 32.4730 to 43.2688 deg
Loaded 4579 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): 3468 out of 3575 total matches.
Matched with Tycho-2 3575 out of 6969 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits:
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits (aperture=6.5)
Read 5741 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1593 to 223.3258 deg, Dec +32.4730 to +43.2527 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 202.1593 to 223.3258 deg, Dec 32.4730 to 43.2527 deg
Loaded 4565 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): 3469 out of 3554 total matches.
Matched with Tycho-2 3554 out of 5741 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits:
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
2.3 pix Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.3 pix fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
2.3 pix fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
2.3 pix wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
2.3 pix wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Limiting magnitude estimates:
15.5 mag. Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
15.3 mag. Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
13.1 mag. fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
12.9 mag. fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.79ffH4cBpu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits' -> 'wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=360, passed=6969
Got 6969 stars (including 6597 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
util/solve_plate_with_UCAC5 got 6969 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
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits N_match=972 sigma_overall_arcsec=0.436 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.503 n_q1=249 n_q2=222 n_q3=245 n_q4=256 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits -region wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.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.SeWRYn0Q9K (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=296, passed=5741
Got 5741 stars (including 5440 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
util/solve_plate_with_UCAC5 got 5741 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=972 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.380 sigma_q4_arcsec=0.432 n_q1=255 n_q2=217 n_q3=248 n_q4=252 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IiBSqV0BcE (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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=85, passed=1581
Got 1581 stars (including 1492 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 1581 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1546 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits N_match=967 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.400 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.299 n_q1=245 n_q2=182 n_q3=364 n_q4=176 worst_quadrant_to_overall_ratio=1.265
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits -region wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.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.uMEqmpy2dd (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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=71, passed=1242
Got 1242 stars (including 1169 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat
util/solve_plate_with_UCAC5 got 1242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 1228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 1228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 1228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits N_match=963 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.331 n_q1=248 n_q2=227 n_q3=282 n_q4=206 worst_quadrant_to_overall_ratio=1.005
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits -region wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits sigma_overall=0.436 worst_q_ratio=1.154
ref2=Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits sigma_overall=0.393 worst_q_ratio=1.202
new1=fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits sigma_overall=0.317 worst_q_ratio=1.265
new2=fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits sigma_overall=0.343 worst_q_ratio=1.005
reference average sigma_overall=0.4145 worst_q_ratio=1.178
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297_astrometric_residuals.png (972 matched stars from wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621_astrometric_residuals.png (972 matched stars from wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080_astrometric_residuals.png (967 matched stars from wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081_astrometric_residuals.png (963 matched stars from wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits'
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits'
Preparing the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Creating symlink local_wcs_cache/wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits exists and is non-empty
wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits exists and is non-empty
wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits exists and is non-empty
wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits (1st reference image)
verification OK: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:10:53.396 +38:00:25.91 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits (1st new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:11:10.804 +38:03:28.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:10:53.396 +38:00:25.91
Second-epoch image center 14:11:10.804 +38:03:28.14
Angular distance between the image centers 0.0763 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits (2nd new image)
verification OK: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:11:11.444 +38:03:05.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:10:53.396 +38:00:25.91
Second-epoch image center 14:11:11.444 +38:03:05.61
Angular distance between the image centers 0.0740 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 14:11:10.804 +38:03:28.14
Second-epoch second image center 14:11:11.444 +38:03:05.61
Angular distance between the image centers 0.00660 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits &> /tmp/tmp.sWltyGqkSY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits &> /tmp/tmp.5iFwMUcwRJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits &> /tmp/tmp.WZ4njpQ26g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits &> /tmp/tmp.wnlLJTsiiO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
Found non-empty wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits and wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
The reference image (wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits) and catalog (wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat) found
'wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat' -> 'wcsmag.cat'
Read 33828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1591 to 223.3611 deg, Dec +32.4150 to +43.2703 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 202.1591 to 223.3611 deg, Dec 32.4150 to 43.2703 deg
Loaded 4612 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): 3303 out of 3579 total matches.
Matched with Tycho-2 3579 out of 33828 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.633000
a=0.000000 b=1.000000 c=22.633000
From vast_summary.log: estimated ref. image limiting mag.: -6.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.69
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1591 to 223.3611 deg, Dec +32.4150 to +43.2703 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 202.1591 to 223.3611 deg, Dec 32.4150 to 43.2703 deg
Loaded 4612 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): 3303 out of 3579 total matches.
Matched with Tycho-2 3579 out of 33828 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits:
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits (aperture=5.1)
Read 29344 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 202.1592 to 223.3842 deg, Dec +32.4482 to +43.2802 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 202.1592 to 223.3842 deg, Dec 32.4482 to 43.2802 deg
Loaded 4599 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): 3321 out of 3583 total matches.
Matched with Tycho-2 3583 out of 29344 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits:
Forced-photometry filter: calibrated wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -> calib.txt_param_ref_wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 169 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
2.2 pix Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
2.2 pix fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
2.2 pix fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
2.2 pix wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
2.2 pix wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Limiting magnitude estimates:
15.7 mag. Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
15.4 mag. Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
13.3 mag. fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
13.1 mag. fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sWltyGqkSY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits' -> 'wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=1418, passed=33801
Got 33801 stars (including 32351 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat
util/solve_plate_with_UCAC5 got 33801 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
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 33401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 33400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 33400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits N_match=973 sigma_overall_arcsec=0.454 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.494 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.491 n_q1=251 n_q2=224 n_q3=241 n_q4=257 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits -region wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.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.5iFwMUcwRJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits' -> 'wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS_IMAGE_NAME=wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS-calibrated image found: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
Checking if the catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits alredy exist and is non-empty...
Catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat corresponding to the image wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits
WCS catalog name: wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1045, passed=29330
Got 29330 stars (including 28250 good ones) from the SExtractor catalog wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat
util/solve_plate_with_UCAC5 got 29330 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 29020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 29020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 29020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits N_match=972 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.458 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.462 n_q1=258 n_q2=225 n_q3=238 n_q4=251 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits -region wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WZ4njpQ26g (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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=216, passed=10954
Got 10954 stars (including 10713 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 10954 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 10783 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 10784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 10784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits N_match=966 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.391 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.311 n_q1=253 n_q2=180 n_q3=358 n_q4=175 worst_quadrant_to_overall_ratio=1.254
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits -region wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.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.wnlLJTsiiO (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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS_IMAGE_NAME=wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS-calibrated image found: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Checking if the catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat corresponding to the image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
WCS catalog name: wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=157, passed=9131
Got 9131 stars (including 8954 good ones) from the SExtractor catalog wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat
util/solve_plate_with_UCAC5 got 9131 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 9035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.0 to 43.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 9033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 9033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits N_match=963 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.348 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.345 n_q1=251 n_q2=228 n_q3=281 n_q4=203 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits -region wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-07_20.00sec_-0.00C_LIGHTs_0080.fits
Saving fully-calibrated image wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.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_2026-06-14_CI_Boo-04-Q1b1x1_232836_TTUQ1b1x1_2121452_0O9ekPwd/wcs_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081.fits
Preparing the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:24.85 +42:23:14.4: 12.00 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:08.31 +39:24:19.0: 11.49 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:14:31.42 +39:15:21.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:41.56 +33:56:14.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:36.92 +33:03:40.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:58.30 +32:58:24.2: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:24.85 +42:23:14.4: 12.00 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:08.31 +39:24:19.0: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 14:45:24.85 +42:23:14.4: ref_mag=12.00 +/- 0.01 new_mean_mag=12.1464 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Forced photometry filter REJECTED candidate at 14:42:08.31 +39:24:19.0: ref_mag=11.49 +/- 0.00 new_mean_mag=11.5414 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:32.83 +35:00:24.8: 13.44 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:41.93 +32:44:48.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:08.44 +34:03:57.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:14:31.42 +39:15:21.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter REJECTED candidate at 14:14:31.42 +39:15:21.0: ref_mag=12.86 +/- 0.01 new_mean_mag=12.7432 delta=0.12 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:36.92 +33:03:40.9: 13.48 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:41.56 +33:56:14.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 14:38:36.92 +33:03:40.9: ref_mag=13.39 +/- 0.03 new_mean_mag=12.4162 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 14:45:41.56 +33:56:14.9: ref_mag=13.59 +/- 0.03 new_mean_mag=12.4905 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:58.30 +32:58:24.2: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 14:38:58.30 +32:58:24.2: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1815 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:41.93 +32:44:48.0: 13.55 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:32.83 +35:00:24.8: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 14:38:41.93 +32:44:48.0: ref_mag=13.45 +/- 0.03 new_mean_mag=12.4289 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 14:47:32.83 +35:00:24.8: ref_mag=13.45 +/- 0.03 new_mean_mag=12.5066 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:08.44 +34:03:57.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:08.44 +34:03:57.7: ref_mag=13.42 +/- 0.03 new_mean_mag=12.5025 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:37:47.77 +34:53:56.4: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:05.29 +33:40:44.3: 13.67 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:51.32 +34:17:46.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:22.54 +33:36:18.1: 14.00 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:47.77 +34:53:56.4: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 14:37:47.77 +34:53:56.4: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4982 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:05.29 +33:40:44.3: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 14:47:05.29 +33:40:44.3: ref_mag=13.71 +/- 0.04 new_mean_mag=12.6334 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:51.32 +34:17:46.9: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 14:41:51.32 +34:17:46.9: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6928 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:22.54 +33:36:18.1: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:22.54 +33:36:18.1: ref_mag=13.98 +/- 0.04 new_mean_mag=12.8983 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.36 +34:32:53.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:02.79 +34:17:52.0: 13.49 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.36 +34:32:53.4: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 14:46:18.36 +34:32:53.4: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6327 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:02.79 +34:17:52.0: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 14:38:02.79 +34:17:52.0: ref_mag=13.46 +/- 0.03 new_mean_mag=12.5029 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.89 +34:17:09.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:07.69 +33:20:04.1: 13.50 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.89 +34:17:09.6: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 14:46:18.89 +34:17:09.6: ref_mag=13.51 +/- 0.03 new_mean_mag=12.5138 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:07.69 +33:20:04.1: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 14:31:07.69 +33:20:04.1: ref_mag=13.52 +/- 0.03 new_mean_mag=12.5781 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:09.09 +32:47:43.7: 12.53 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:09.09 +32:47:43.7: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 14:38:09.09 +32:47:43.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5881 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:23.91 +33:26:36.0: 12.53 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:23.91 +33:26:36.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 14:39:23.91 +33:26:36.0: ref_mag=12.54 +/- 0.01 new_mean_mag=11.6098 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:51.66 +32:44:59.7: 12.55 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:49.42 +32:55:42.7: 14.24 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:51.66 +32:44:59.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:58.35 +34:28:17.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 14:40:51.66 +32:44:59.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5602 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:49.42 +32:55:42.7: 14.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.06
Forced photometry filter KEPT candidate at 14:39:49.42 +32:55:42.7: ref_mag=14.28 +/- 0.06 new_mean_mag=13.0606 delta=1.22 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:58.35 +34:28:17.5: 13.36 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:35.46 +33:31:52.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:58.35 +34:28:17.5: ref_mag=13.33 +/- 0.03 new_mean_mag=12.4140 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:35.46 +33:31:52.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 14:42:35.46 +33:31:52.6: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6908 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:06.28 +33:18:57.0: 13.71 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:06.28 +33:18:57.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 14:39:06.28 +33:18:57.0: ref_mag=13.71 +/- 0.03 new_mean_mag=12.6413 delta=1.07 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:19.70 +34:44:54.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:19.70 +34:44:54.8: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:19.70 +34:44:54.8: ref_mag=13.55 +/- 0.03 new_mean_mag=12.5965 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:36.27 +34:01:24.2: 12.71 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:36.27 +34:01:24.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 14:41:36.27 +34:01:24.2: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7779 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:36.44 +33:27:30.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:36.44 +33:27:30.7: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 14:44:36.44 +33:27:30.7: ref_mag=13.79 +/- 0.04 new_mean_mag=12.6110 delta=1.18 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:05.44 +33:03:53.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:06.07 +34:19:01.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:05.44 +33:03:53.4: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:05.44 +33:03:53.4: ref_mag=13.74 +/- 0.04 new_mean_mag=12.7960 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:06.07 +34:19:01.8: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 14:44:06.07 +34:19:01.8: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7591 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:08.60 +34:13:57.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:08.60 +34:13:57.0: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter KEPT candidate at 14:43:08.60 +34:13:57.0: ref_mag=13.80 +/- 0.04 new_mean_mag=12.6729 delta=1.13 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:43.22 +33:04:52.1: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:43.22 +33:04:52.1: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 14:43:43.22 +33:04:52.1: ref_mag=13.78 +/- 0.04 new_mean_mag=12.6871 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:47.35 +33:50:08.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:46.91 +33:42:17.2: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:29.80 +33:13:49.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:47.35 +33:50:08.0: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 14:38:47.35 +33:50:08.0: ref_mag=12.98 +/- 0.02 new_mean_mag=12.0416 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:46.91 +33:42:17.2: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:29.80 +33:13:49.2: 13.04 +/- 0.03 detection
Forced photometry filter KEPT candidate at 14:43:46.91 +33:42:17.2: ref_mag=13.64 +/- 0.03 new_mean_mag=12.6147 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 14:39:29.80 +33:13:49.2: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0136 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:43.91 +32:58:42.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:43.91 +32:58:42.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 14:31:43.91 +32:58:42.6: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1058 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:28.10 +33:49:23.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:28.10 +33:49:23.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 14:45:28.10 +33:49:23.4: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0960 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:41.03 +33:57:01.9: 13.03 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:41.03 +33:57:01.9: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 14:46:41.03 +33:57:01.9: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0823 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:37.97 +33:10:01.8: 13.02 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:37.97 +33:10:01.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 14:38:37.97 +33:10:01.8: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0442 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:12.27 +34:00:50.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:12.27 +34:00:50.5: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 14:42:12.27 +34:00:50.5: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0397 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:37.70 +33:13:08.2: 13.94 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:37.70 +33:13:08.2: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 14:44:37.70 +33:13:08.2: ref_mag=13.94 +/- 0.04 new_mean_mag=12.7707 delta=1.17 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:38.21 +34:56:25.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:38.13 +34:39:34.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:38.21 +34:56:25.9: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 14:38:38.21 +34:56:25.9: ref_mag=13.59 +/- 0.03 new_mean_mag=12.6173 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:38.13 +34:39:34.9: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 14:44:38.13 +34:39:34.9: ref_mag=13.57 +/- 0.03 new_mean_mag=12.5864 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:21.50 +32:42:29.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:21.50 +32:42:29.1: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:21.50 +32:42:29.1: ref_mag=13.94 +/- 0.04 new_mean_mag=12.8375 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:14.26 +33:07:35.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:54.02 +32:49:21.7: 14.12 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:14.26 +33:07:35.3: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:14.26 +33:07:35.3: ref_mag=13.59 +/- 0.03 new_mean_mag=12.4988 delta=1.09 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:54.02 +32:49:21.7: 14.21 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry filter KEPT candidate at 14:43:54.02 +32:49:21.7: ref_mag=14.15 +/- 0.06 new_mean_mag=12.9838 delta=1.16 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:56.04 +32:46:01.1: 13.55 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:56.04 +32:46:01.1: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 14:38:56.04 +32:46:01.1: ref_mag=13.60 +/- 0.03 new_mean_mag=12.5846 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:40.12 +34:06:19.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:40.12 +34:06:19.0: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 14:45:40.12 +34:06:19.0: ref_mag=13.88 +/- 0.04 new_mean_mag=12.7469 delta=1.14 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:00.82 +32:59:49.8: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:00.82 +32:59:49.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 14:40:00.82 +32:59:49.8: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7777 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:19.07 +33:50:39.5: 13.77 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:19.07 +33:50:39.5: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 14:45:19.07 +33:50:39.5: ref_mag=13.79 +/- 0.04 new_mean_mag=12.6670 delta=1.12 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:25.67 +33:04:03.3: 14.24 +/- 0.08 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:25.67 +33:04:03.3: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry filter KEPT candidate at 14:44:25.67 +33:04:03.3: ref_mag=14.18 +/- 0.06 new_mean_mag=12.9159 delta=1.26 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:20.67 +33:35:20.7: 12.30 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:20.67 +33:35:20.7: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 14:45:20.67 +33:35:20.7: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3384 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:27.30 +33:34:33.7: 13.52 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:27.30 +33:34:33.7: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:27.30 +33:34:33.7: ref_mag=13.56 +/- 0.03 new_mean_mag=12.4443 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:21.14 +35:19:44.3: 13.88 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:21.14 +35:19:44.3: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Forced photometry filter KEPT candidate at 14:47:21.14 +35:19:44.3: ref_mag=13.91 +/- 0.04 new_mean_mag=12.9015 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:14.37 +34:10:10.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:14.37 +34:10:10.8: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 14:41:14.37 +34:10:10.8: ref_mag=13.79 +/- 0.04 new_mean_mag=12.7423 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:51.93 +33:37:42.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:51.93 +33:37:42.1: 14.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 14:40:51.93 +33:37:42.1: ref_mag=14.10 +/- 0.05 new_mean_mag=12.8431 delta=1.26 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:18.85 +33:35:24.2: 12.99 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:18.85 +33:35:24.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 14:46:18.85 +33:35:24.2: ref_mag=13.01 +/- 0.02 new_mean_mag=11.9571 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:14.73 +33:08:23.9: 13.54 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:14.73 +33:08:23.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 14:30:14.73 +33:08:23.9: ref_mag=13.60 +/- 0.03 new_mean_mag=12.6551 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:05.73 +32:54:06.9: 13.87 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:05.73 +32:54:06.9: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter KEPT candidate at 14:39:05.73 +32:54:06.9: ref_mag=13.89 +/- 0.04 new_mean_mag=12.7787 delta=1.11 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:57.23 +33:54:23.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:57.23 +33:54:23.5: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 14:38:57.23 +33:54:23.5: ref_mag=13.82 +/- 0.04 new_mean_mag=12.7483 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:31.57 +33:39:04.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:31.57 +33:39:04.5: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:31.57 +33:39:04.5: ref_mag=13.70 +/- 0.03 new_mean_mag=12.5640 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:31.97 +35:36:12.3: 13.51 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:31.97 +35:36:12.3: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 14:44:31.97 +35:36:12.3: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6353 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:03.20 +33:55:57.0: 13.74 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:03.20 +33:55:57.0: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 14:47:03.20 +33:55:57.0: ref_mag=13.71 +/- 0.04 new_mean_mag=12.6350 delta=1.07 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:26.80 +32:48:05.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:26.80 +32:48:05.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 14:38:26.80 +32:48:05.0: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0316 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:20.22 +33:38:09.5: 12.96 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:20.22 +33:38:09.5: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 14:40:20.22 +33:38:09.5: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9221 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:12.83 +32:50:49.8: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:00.28 +33:31:51.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:12.83 +32:50:49.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:12.83 +32:50:49.8: ref_mag=13.86 +/- 0.04 new_mean_mag=12.6208 delta=1.23 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:00.28 +33:31:51.8: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 14:44:00.28 +33:31:51.8: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9839 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:26.95 +32:54:47.6: 11.40 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:26.95 +32:54:47.6: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Forced photometry filter KEPT candidate at 14:41:26.95 +32:54:47.6: ref_mag=11.42 +/- 0.00 new_mean_mag=10.4862 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:54.62 +34:16:35.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:54.62 +34:16:35.6: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 14:45:54.62 +34:16:35.6: ref_mag=13.35 +/- 0.03 new_mean_mag=12.3373 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:19.70 +33:49:51.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:19.70 +33:49:51.2: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:19.70 +33:49:51.2: ref_mag=13.52 +/- 0.03 new_mean_mag=12.5738 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:09.13 +34:19:08.3: 13.32 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:09.13 +34:19:08.3: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 14:42:09.13 +34:19:08.3: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4129 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:41.81 +33:16:28.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:41.81 +33:16:28.0: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 14:45:41.81 +33:16:28.0: ref_mag=13.38 +/- 0.03 new_mean_mag=12.2088 delta=1.17 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:15.10 +33:13:53.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:15.10 +33:13:53.4: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 14:30:15.10 +33:13:53.4: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3062 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:13.71 +32:52:10.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:53.18 +33:17:19.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:13.71 +32:52:10.4: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 14:41:13.71 +32:52:10.4: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6167 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:53.18 +33:17:19.5: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Forced photometry filter KEPT candidate at 14:43:53.18 +33:17:19.5: ref_mag=14.06 +/- 0.05 new_mean_mag=12.8300 delta=1.23 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:38:40.15 +33:25:18.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:38:40.15 +33:25:18.8: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 14:38:40.15 +33:25:18.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.7122 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:59.09 +33:26:07.0: 12.56 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:59.09 +33:26:07.0: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 14:45:59.09 +33:26:07.0: ref_mag=12.58 +/- 0.01 new_mean_mag=11.5396 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:41.28 +33:16:00.6: 12.56 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:47.00 +33:23:30.3: 14.12 +/- 0.07 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:41.28 +33:16:00.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 14:41:41.28 +33:16:00.6: ref_mag=12.58 +/- 0.01 new_mean_mag=11.5961 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:47.00 +33:23:30.3: 14.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Forced photometry filter KEPT candidate at 14:46:47.00 +33:23:30.3: ref_mag=14.12 +/- 0.06 new_mean_mag=12.9647 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:55.98 +32:56:36.8: 14.21 +/- 0.08 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:55.98 +32:56:36.8: 14.16 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter KEPT candidate at 14:42:55.98 +32:56:36.8: ref_mag=14.19 +/- 0.06 new_mean_mag=12.9986 delta=1.19 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:39.43 +32:50:36.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:39.43 +32:50:36.8: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 14:43:39.43 +32:50:36.8: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2552 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:22.45 +32:57:09.8: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:22.45 +32:57:09.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 14:29:22.45 +32:57:09.8: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3130 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:48:21.86 +35:32:14.3: 13.71 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:48:21.86 +35:32:14.3: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 14:48:21.86 +35:32:14.3: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7376 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:19.53 +33:50:46.4: 12.89 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:19.53 +33:50:46.4: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 14:40:19.53 +33:50:46.4: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9952 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:30.21 +33:41:19.6: 13.49 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:06.19 +34:11:31.7: 13.48 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:06.19 +34:11:31.7: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 14:46:06.19 +34:11:31.7: ref_mag=13.47 +/- 0.03 new_mean_mag=12.4381 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:30.21 +33:41:19.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:30.21 +33:41:19.6: ref_mag=13.54 +/- 0.03 new_mean_mag=12.5153 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:24.88 +34:26:50.8: 13.70 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:24.88 +34:26:50.8: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 14:47:24.88 +34:26:50.8: ref_mag=13.71 +/- 0.04 new_mean_mag=12.6958 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:41.55 +33:18:44.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:41.55 +33:18:44.0: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 14:39:41.55 +33:18:44.0: ref_mag=13.51 +/- 0.03 new_mean_mag=12.5097 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:19.41 +34:36:45.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:19.41 +34:36:45.4: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 14:47:19.41 +34:36:45.4: ref_mag=13.49 +/- 0.03 new_mean_mag=12.4079 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:00.41 +32:52:38.2: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:30:35.86 +32:51:27.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:30:35.86 +32:51:27.7: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 14:30:35.86 +32:51:27.7: ref_mag=13.50 +/- 0.03 new_mean_mag=12.3896 delta=1.12 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:00.41 +32:52:38.2: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:00.41 +32:52:38.2: ref_mag=13.48 +/- 0.03 new_mean_mag=12.2862 delta=1.20 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:36.97 +33:24:51.0: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:36.97 +33:24:51.0: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 14:43:36.97 +33:24:51.0: ref_mag=13.88 +/- 0.04 new_mean_mag=12.8453 delta=1.04 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:13.55 +32:59:16.1: 13.86 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:13.55 +32:59:16.1: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:13.55 +32:59:16.1: ref_mag=13.90 +/- 0.04 new_mean_mag=12.8938 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:09.33 +33:26:17.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:09.33 +33:26:17.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 14:31:09.33 +33:26:17.8: ref_mag=13.48 +/- 0.03 new_mean_mag=12.5441 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:35.14 +33:33:19.0: 12.13 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:35.14 +33:33:19.0: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter KEPT candidate at 14:46:35.14 +33:33:19.0: ref_mag=12.16 +/- 0.01 new_mean_mag=11.1657 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:34.03 +33:03:30.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:34.03 +33:03:30.4: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 14:40:34.03 +33:03:30.4: ref_mag=13.94 +/- 0.04 new_mean_mag=12.8835 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:56.40 +33:22:17.8: 12.52 +/- 0.02 detection
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:36.11 +33:15:57.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:56.40 +33:22:17.8: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 14:42:56.40 +33:22:17.8: ref_mag=12.55 +/- 0.01 new_mean_mag=11.5522 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:36.11 +33:15:57.6: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 14:29:36.11 +33:15:57.6: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3375 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:05.31 +33:32:48.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:52.59 +33:30:38.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:05.31 +33:32:48.3: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 14:44:05.31 +33:32:48.3: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2405 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:52.59 +33:30:38.0: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 14:42:52.59 +33:30:38.0: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2254 delta=1.01 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:33.81 +34:42:17.6: 13.66 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:33.81 +34:42:17.6: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 14:41:33.81 +34:42:17.6: ref_mag=13.64 +/- 0.03 new_mean_mag=12.7044 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:58.12 +33:16:33.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:58.12 +33:16:33.8: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:58.12 +33:16:33.8: ref_mag=13.64 +/- 0.03 new_mean_mag=12.4997 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:59.90 +33:25:05.9: 13.67 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:59.90 +33:25:05.9: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 14:43:59.90 +33:25:05.9: ref_mag=13.75 +/- 0.04 new_mean_mag=12.6525 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:57.74 +32:44:27.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:57.74 +32:44:27.4: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:57.74 +32:44:27.4: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6246 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:44.70 +32:55:38.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:44.70 +32:55:38.9: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 14:31:44.70 +32:55:38.9: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2288 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:39:02.52 +33:25:56.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:39:02.52 +33:25:56.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 14:39:02.52 +33:25:56.4: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2833 delta=0.93 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:27.70 +32:57:35.5: 13.17 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:27.70 +32:57:35.5: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 14:31:27.70 +32:57:35.5: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2638 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:30.34 +33:10:00.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:30.34 +33:10:00.4: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 14:44:30.34 +33:10:00.4: ref_mag=12.85 +/- 0.02 new_mean_mag=11.7558 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:58.89 +33:28:12.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:58.89 +33:28:12.5: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:58.89 +33:28:12.5: ref_mag=13.46 +/- 0.03 new_mean_mag=12.4096 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:47.87 +33:25:58.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:47.87 +33:25:58.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 14:41:47.87 +33:25:58.9: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8731 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:49.41 +33:21:10.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:49.41 +33:21:10.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 14:41:49.41 +33:21:10.2: ref_mag=12.50 +/- 0.01 new_mean_mag=11.5528 delta=0.95 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:49.30 +33:34:58.9: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:49.30 +33:34:58.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 14:45:49.30 +33:34:58.9: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1396 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:58.15 +33:59:55.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:58.15 +33:59:55.7: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 14:44:58.15 +33:59:55.7: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1939 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:17.05 +32:45:04.6: 12.78 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:17.05 +32:45:04.6: 12.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter REJECTED candidate at 14:40:17.05 +32:45:04.6: ref_mag=12.78 +/- 0.02 new_mean_mag=12.0898 delta=0.69 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:32.35 +33:37:47.2: 12.47 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:32.35 +33:37:47.2: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 14:42:32.35 +33:37:47.2: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5597 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:06.38 +32:53:18.9: 11.98 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:06.38 +32:53:18.9: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 14:42:06.38 +32:53:18.9: ref_mag=12.01 +/- 0.01 new_mean_mag=11.0368 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:44:39.56 +33:44:37.7: 13.42 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:44:39.56 +33:44:37.7: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 14:44:39.56 +33:44:37.7: ref_mag=13.46 +/- 0.03 new_mean_mag=12.4655 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:03.76 +33:30:32.3: 13.41 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:03.76 +33:30:32.3: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 14:40:03.76 +33:30:32.3: ref_mag=13.44 +/- 0.03 new_mean_mag=12.4320 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:29:44.53 +32:56:51.9: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:29:44.53 +32:56:51.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 14:29:44.53 +32:56:51.9: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3931 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:37:53.69 +34:59:24.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:04.32 +32:43:16.8: 13.39 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:37:53.69 +34:59:24.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 14:37:53.69 +34:59:24.0: ref_mag=13.45 +/- 0.02 new_mean_mag=12.2915 delta=1.16 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:48.74 +33:05:59.7: 13.13 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:04.32 +32:43:16.8: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 14:41:04.32 +32:43:16.8: ref_mag=13.36 +/- 0.03 new_mean_mag=12.3181 delta=1.05 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:48.74 +33:05:59.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 14:41:48.74 +33:05:59.7: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1260 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:41:03.71 +33:44:36.0: 13.64 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:12.48 +32:45:33.9: 13.78 +/- 0.05 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:41:03.71 +33:44:36.0: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 14:41:03.71 +33:44:36.0: ref_mag=13.66 +/- 0.03 new_mean_mag=12.6703 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:12.48 +32:45:33.9: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 14:43:12.48 +32:45:33.9: ref_mag=13.79 +/- 0.04 new_mean_mag=12.6694 delta=1.12 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:28.51 +32:57:54.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:28.51 +32:57:54.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 14:40:28.51 +32:57:54.7: ref_mag=12.83 +/- 0.02 new_mean_mag=11.8503 delta=0.98 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:45.04 +33:35:08.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:45.04 +33:35:08.0: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 14:43:45.04 +33:35:08.0: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1387 delta=1.02 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:38.21 +34:40:36.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:38.21 +34:40:36.0: 13.14 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:40:20.88 +33:10:15.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 14:45:38.21 +34:40:36.0: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1865 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:40:20.88 +33:10:15.9: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 14:40:20.88 +33:10:15.9: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8730 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:31:04.57 +32:57:28.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:31:04.57 +32:57:28.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 14:31:04.57 +32:57:28.1: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8346 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:43:23.54 +34:32:34.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:43:23.54 +34:32:34.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 14:43:23.54 +34:32:34.0: ref_mag=13.65 +/- 0.03 new_mean_mag=12.5844 delta=1.06 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:46:34.79 +34:16:12.8: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:46:34.79 +34:16:12.8: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter KEPT candidate at 14:46:34.79 +34:16:12.8: ref_mag=13.62 +/- 0.04 new_mean_mag=12.6509 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:47:00.58 +34:21:27.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:47:00.58 +34:21:27.1: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 14:47:00.58 +34:21:27.1: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6192 delta=0.93 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:42:25.43 +33:16:10.6: 13.36 +/- 0.03 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:42:25.43 +33:16:10.6: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 14:42:25.43 +33:16:10.6: ref_mag=13.35 +/- 0.03 new_mean_mag=12.3507 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-11_01-51-25_20.00sec_-5.00C_LIGHT_0297.fits at 14:45:39.19 +32:57:44.3: 12.36 +/- 0.01 detection
Forced photometry on wcs_Boo-04-Q1b1x1_2026-05-18_01-39-59_20.00sec_5.00C_LIGHT_1621.fits at 14:45:39.19 +32:57:44.3: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 14:45:39.19 +32:57:44.3: ref_mag=12.38 +/- 0.01 new_mean_mag=11.3178 delta=1.06 (need > 0.90)
Adding exclusion_list_local.txt__out21043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24971.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out25047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25343.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out25454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25530.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out25539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25580.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out25649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27205.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out27419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27469.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out27586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27603.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out27935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28456.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out28549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31915.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 166s
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: 64s
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Considering the candidate 50955_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 50955_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 13:34:53.28 +33:13:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50989_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 50989_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
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Considering the candidate 51082_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 51082_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
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Considering the candidate 51145_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 51145_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 13:44:08.12 +42:44:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51225_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 51225_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
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Considering the candidate 51263_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 51263_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 13:49:50.23 +36:35:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21989_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21989_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 26684_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26684_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21760_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21760_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21756_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21756_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:09.84 +33:00:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26715_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26715_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 30266_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 30266_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21078_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21078_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22938_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 22938_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:12.35 +33:24:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21045_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21045_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:33:44.00 +32:47:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29412_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29412_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25814_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25814_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:38:31.71 +33:46:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25947_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25947_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 27603_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27603_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25343_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25343_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21789_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21789_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:25.38 +33:02:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25359_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25359_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:33:03.61 +33:42:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27935_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27935_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 27419_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27419_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 27818_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27818_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22525_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22525_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21194_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21194_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 24706_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24706_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21171_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21171_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21680_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21680_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 28305_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28305_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25206_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25206_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25686_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25686_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:13.99 +33:45:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22778_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22778_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25667_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25667_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:49.86 +33:45:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29098_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29098_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 26768_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26768_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25114_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25114_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22065_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22065_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 27833_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27833_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 27469_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27469_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22294_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22294_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 26010_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26010_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22527_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22527_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25628_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25628_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21515_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21515_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 26298_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26298_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25839_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25839_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:38:20.81 +33:46:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25271_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25271_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:33:39.41 +33:41:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26574_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26574_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22314_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22314_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 26704_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26704_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22740_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22740_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 24879_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 24879_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:38:22.97 +33:29:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29595_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29595_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 28960_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28960_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21493_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21493_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:35:51.66 +32:55:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21043_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21043_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 22260_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22260_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21550_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21550_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21316_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21316_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:33:54.71 +32:53:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26033_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 26033_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:55.98 +33:52:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21138_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21138_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25037_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25037_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:34:43.71 +33:39:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22220_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 22220_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:38:12.27 +33:08:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27194_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27194_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 21858_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21858_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26412_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26412_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22289_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22289_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25539_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25539_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 25361_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25361_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31304_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 31304_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27205_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27205_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28791_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28791_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25580_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25580_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21921_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21921_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25731_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 25731_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:34:59.70 +33:47:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21564_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21564_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26195_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26195_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 29097_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29097_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31915_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 31915_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27226_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27226_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21228_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21228_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25468_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25468_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21453_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21453_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25257_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25257_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21689_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21689_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27541_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27541_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26214_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26214_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27557_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27557_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22970_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22970_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22196_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22196_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22306_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 22306_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:34:55.18 +33:12:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28955_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 28955_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:35:24.30 +34:46:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26262_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 26262_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:58.49 +33:56:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22051_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 22051_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:33:43.59 +33:08:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21554_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21554_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22925_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22925_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24684_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24684_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21796_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21796_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:19.01 +33:01:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25078_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25078_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22734_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22734_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29453_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29453_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21841_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21841_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21593_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21593_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21371_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21371_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31892_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 31892_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26120_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26120_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21895_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21895_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:51.08 +33:02:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25563_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25563_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27586_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27586_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
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Considering the candidate 28549_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28549_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22797_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22797_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28992_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28992_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21525_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21525_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21113_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21113_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24887_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24887_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21846_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21846_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22852_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22852_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28456_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28456_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22067_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22067_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24695_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24695_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22287_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22287_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24978_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 24978_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:32:41.01 +33:35:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25362_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25362_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25047_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25047_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29005_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29005_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22717_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22717_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24833_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24833_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21150_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21150_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21366_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21366_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24723_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24723_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21455_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21455_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22526_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 22526_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:31.73 +33:15:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22569_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22569_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25013_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25013_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24908_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24908_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21223_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21223_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:35:13.49 +32:50:31.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26329_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 26329_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:38:27.72 +33:57:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22998_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22998_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21429_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21429_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:34:00.15 +32:55:19.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25535_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25535_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26880_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26880_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21148_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21148_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25530_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25530_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21644_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21644_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26011_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 26011_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24971_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 24971_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21358_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21358_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29664_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29664_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21104_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21104_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22246_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22246_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25649_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25649_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21318_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21318_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21799_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21799_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25454_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 25454_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29123_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 29123_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21867_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21867_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:42.44 +33:02:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22382_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22382_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21440_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 21440_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21407_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21407_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:36:57.75 +32:52:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28535_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28535_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27859_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 27859_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28168_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 28168_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22789_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22789_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22023_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
Preparing report for the candidate 22023_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21147_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 21147_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 14:37:11.05 +32:47:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33581_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 33581_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 13:37:27.58 +36:17:43.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18244_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081
The candidate 18244_fd_Boo-04-Q1b1x1_2026-06-14_22-58-44_20.00sec_0.00C_LIGHTs_0081 did not pass the final checks
**** FOUND 13:34:48.13 +37:10:57.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 238s
Prepared the HTML report for the field Boo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:40:21.50 +32:42:29.1
14:38:41.93 +32:44:48.0
14:41:04.32 +32:43:16.8
14:30:35.86 +32:51:27.7
14:38:56.04 +32:46:01.1
14:40:57.74 +32:44:27.4
14:40:51.66 +32:44:59.7
14:38:09.09 +32:47:43.7
14:38:26.80 +32:48:05.0
14:43:12.48 +32:45:33.9
14:29:44.53 +32:56:51.9
14:31:44.70 +32:55:38.9
14:29:22.45 +32:57:09.8
14:31:04.57 +32:57:28.1
14:40:12.83 +32:50:49.8
14:31:27.70 +32:57:35.5
14:31:43.91 +32:58:42.6
14:40:00.41 +32:52:38.2
14:43:54.02 +32:49:21.7
14:41:13.71 +32:52:10.4
14:39:05.73 +32:54:06.9
14:43:39.43 +32:50:36.8
14:42:06.38 +32:53:18.9
14:39:49.42 +32:55:42.7
14:41:26.95 +32:54:47.6
14:38:58.30 +32:58:24.2
14:40:28.51 +32:57:54.7
14:42:55.98 +32:56:36.8
14:40:13.55 +32:59:16.1
14:40:00.82 +32:59:49.8
14:30:14.73 +33:08:23.9
14:38:36.92 +33:03:40.9
14:45:39.19 +32:57:44.3
14:40:05.44 +33:03:53.4
14:40:34.03 +33:03:30.4
14:30:15.10 +33:13:53.4
14:41:48.74 +33:05:59.7
14:40:14.26 +33:07:35.3
14:29:36.11 +33:15:57.6
14:44:25.67 +33:04:03.3
14:43:43.22 +33:04:52.1
14:38:37.97 +33:10:01.8
14:40:20.88 +33:10:15.9
14:31:07.69 +33:20:04.1
14:39:29.80 +33:13:49.2
14:44:30.34 +33:10:00.4
14:40:58.12 +33:16:33.8
14:41:41.28 +33:16:00.6
14:44:37.70 +33:13:08.2
14:39:06.28 +33:18:57.0
14:42:25.43 +33:16:10.6
14:39:41.55 +33:18:44.0
14:31:09.33 +33:26:17.8
14:43:53.18 +33:17:19.5
14:45:41.81 +33:16:28.0
14:41:49.41 +33:21:10.2
14:38:40.15 +33:25:18.8
14:42:56.40 +33:22:17.8
14:39:23.91 +33:26:36.0
14:39:02.52 +33:25:56.4
14:43:59.90 +33:25:05.9
14:43:36.97 +33:24:51.0
14:41:47.87 +33:25:58.9
14:40:03.76 +33:30:32.3
14:42:58.89 +33:28:12.5
14:42:52.59 +33:30:38.0
14:45:59.09 +33:26:07.0
14:44:36.44 +33:27:30.7
14:42:35.46 +33:31:52.6
14:44:00.28 +33:31:51.8
14:40:22.54 +33:36:18.1
14:42:27.30 +33:34:33.7
14:44:05.31 +33:32:48.3
14:43:45.04 +33:35:08.0
14:40:20.22 +33:38:09.5
14:42:32.35 +33:37:47.2
14:45:49.30 +33:34:58.9
14:45:20.67 +33:35:20.7
14:42:30.21 +33:41:19.6
14:46:18.85 +33:35:24.2
14:43:46.91 +33:42:17.2
14:41:03.71 +33:44:36.0
14:47:05.29 +33:40:44.3
14:38:47.35 +33:50:08.0
14:44:39.56 +33:44:37.7
14:40:19.53 +33:50:46.4
14:38:57.23 +33:54:23.5
14:42:19.70 +33:49:51.2
14:45:28.10 +33:49:23.4
14:45:19.07 +33:50:39.5
14:46:41.03 +33:57:01.9
14:45:41.56 +33:56:14.9
14:42:12.27 +34:00:50.5
14:40:08.44 +34:03:57.7
14:41:36.27 +34:01:24.2
14:44:58.15 +33:59:55.7
14:45:40.12 +34:06:19.0
14:41:14.37 +34:10:10.8
14:47:03.20 +33:55:57.0
14:38:02.79 +34:17:52.0
14:43:08.60 +34:13:57.0
14:45:54.62 +34:16:35.6
14:42:09.13 +34:19:08.3
14:46:06.19 +34:11:31.7
14:41:51.32 +34:17:46.9
14:46:18.89 +34:17:09.6
14:44:06.07 +34:19:01.8
14:46:34.79 +34:16:12.8
14:46:18.36 +34:32:53.4
14:47:00.58 +34:21:27.1
14:42:58.35 +34:28:17.5
14:46:35.14 +33:33:19.0
14:43:23.54 +34:32:34.0
14:47:24.88 +34:26:50.8
14:40:51.93 +33:37:42.1
14:44:38.13 +34:39:34.9
14:47:19.41 +34:36:45.4
14:41:33.81 +34:42:17.6
14:40:31.57 +33:39:04.5
14:40:19.70 +34:44:54.8
14:45:38.21 +34:40:36.0
14:37:47.77 +34:53:56.4
14:46:47.00 +33:23:30.3
14:38:38.21 +34:56:25.9
14:37:53.69 +34:59:24.0
14:47:32.83 +35:00:24.8
14:47:21.14 +35:19:44.3
14:48:21.86 +35:32:14.3
14:44:31.97 +35:36:12.3
########### Completed Boo-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
14:38:36.92 +33:03:40.9
14:45:41.56 +33:56:14.9
14:38:58.30 +32:58:24.2
14:40:08.44 +34:03:57.7
14:47:32.83 +35:00:24.8
14:38:41.93 +32:44:48.0
14:37:47.77 +34:53:56.4
14:47:05.29 +33:40:44.3
14:41:51.32 +34:17:46.9
14:40:22.54 +33:36:18.1
14:46:18.36 +34:32:53.4
14:38:02.79 +34:17:52.0
14:46:18.89 +34:17:09.6
14:31:07.69 +33:20:04.1
14:38:09.09 +32:47:43.7
14:39:23.91 +33:26:36.0
14:40:51.66 +32:44:59.7
14:39:49.42 +32:55:42.7
14:42:58.35 +34:28:17.5
14:42:35.46 +33:31:52.6
14:39:06.28 +33:18:57.0
14:40:19.70 +34:44:54.8
14:41:36.27 +34:01:24.2
14:44:36.44 +33:27:30.7
14:40:05.44 +33:03:53.4
14:44:06.07 +34:19:01.8
14:43:08.60 +34:13:57.0
14:43:43.22 +33:04:52.1
14:38:47.35 +33:50:08.0
14:39:29.80 +33:13:49.2
14:43:46.91 +33:42:17.2
14:31:43.91 +32:58:42.6
14:45:28.10 +33:49:23.4
14:46:41.03 +33:57:01.9
14:38:37.97 +33:10:01.8
14:42:12.27 +34:00:50.5
14:44:37.70 +33:13:08.2
14:38:38.21 +34:56:25.9
14:44:38.13 +34:39:34.9
14:40:21.50 +32:42:29.1
14:40:14.26 +33:07:35.3
14:43:54.02 +32:49:21.7
14:38:56.04 +32:46:01.1
14:45:40.12 +34:06:19.0
14:40:00.82 +32:59:49.8
14:45:19.07 +33:50:39.5
14:44:25.67 +33:04:03.3
14:45:20.67 +33:35:20.7
14:42:27.30 +33:34:33.7
14:47:21.14 +35:19:44.3
14:41:14.37 +34:10:10.8
14:40:51.93 +33:37:42.1
14:46:18.85 +33:35:24.2
14:30:14.73 +33:08:23.9
14:39:05.73 +32:54:06.9
14:38:57.23 +33:54:23.5
14:40:31.57 +33:39:04.5
14:44:31.97 +35:36:12.3
14:47:03.20 +33:55:57.0
14:38:26.80 +32:48:05.0
14:40:20.22 +33:38:09.5
14:40:12.83 +32:50:49.8
14:44:00.28 +33:31:51.8
14:41:26.95 +32:54:47.6
14:45:54.62 +34:16:35.6
14:42:19.70 +33:49:51.2
14:42:09.13 +34:19:08.3
14:45:41.81 +33:16:28.0
14:30:15.10 +33:13:53.4
14:41:13.71 +32:52:10.4
14:43:53.18 +33:17:19.5
14:38:40.15 +33:25:18.8
14:45:59.09 +33:26:07.0
14:41:41.28 +33:16:00.6
14:46:47.00 +33:23:30.3
14:42:55.98 +32:56:36.8
14:43:39.43 +32:50:36.8
14:29:22.45 +32:57:09.8
14:48:21.86 +35:32:14.3
14:40:19.53 +33:50:46.4
14:42:30.21 +33:41:19.6
14:46:06.19 +34:11:31.7
14:47:24.88 +34:26:50.8
14:39:41.55 +33:18:44.0
14:47:19.41 +34:36:45.4
14:40:00.41 +32:52:38.2
14:30:35.86 +32:51:27.7
14:43:36.97 +33:24:51.0
14:40:13.55 +32:59:16.1
14:31:09.33 +33:26:17.8
14:46:35.14 +33:33:19.0
14:40:34.03 +33:03:30.4
14:42:56.40 +33:22:17.8
14:29:36.11 +33:15:57.6
14:44:05.31 +33:32:48.3
14:42:52.59 +33:30:38.0
14:41:33.81 +34:42:17.6
14:40:58.12 +33:16:33.8
14:43:59.90 +33:25:05.9
14:40:57.74 +32:44:27.4
14:31:44.70 +32:55:38.9
14:39:02.52 +33:25:56.4
14:31:27.70 +32:57:35.5
14:44:30.34 +33:10:00.4
14:42:58.89 +33:28:12.5
14:41:47.87 +33:25:58.9
14:41:49.41 +33:21:10.2
14:45:49.30 +33:34:58.9
14:44:58.15 +33:59:55.7
14:42:32.35 +33:37:47.2
14:42:06.38 +32:53:18.9
14:44:39.56 +33:44:37.7
14:40:03.76 +33:30:32.3
14:29:44.53 +32:56:51.9
14:37:53.69 +34:59:24.0
14:41:04.32 +32:43:16.8
14:41:48.74 +33:05:59.7
14:41:03.71 +33:44:36.0
14:43:12.48 +32:45:33.9
14:40:28.51 +32:57:54.7
14:43:45.04 +33:35:08.0
14:45:38.21 +34:40:36.0
14:40:20.88 +33:10:15.9
14:31:04.57 +32:57:28.1
14:43:23.54 +34:32:34.0
14:46:34.79 +34:16:12.8
14:47:00.58 +34:21:27.1
14:42:25.43 +33:16:10.6
14:45:39.19 +32:57:44.3
###################################################################################
14:38:36.92 +33:03:40.9 -- not an asteroid (will add it to exclusion list)
14:45:41.56 +33:56:14.9 -- not an asteroid (will add it to exclusion list)
14:38:58.30 +32:58:24.2 -- not an asteroid (will add it to exclusion list)
14:40:08.44 +34:03:57.7 -- not an asteroid (will add it to exclusion list)
14:47:32.83 +35:00:24.8 -- not an asteroid (will add it to exclusion list)
14:38:41.93 +32:44:48.0 -- not an asteroid (will add it to exclusion list)
14:37:47.77 +34:53:56.4 -- not an asteroid (will add it to exclusion list)
14:47:05.29 +33:40:44.3 -- not an asteroid (will add it to exclusion list)
14:41:51.32 +34:17:46.9 -- not an asteroid (will add it to exclusion list)
14:40:22.54 +33:36:18.1 -- not an asteroid (will add it to exclusion list)
14:46:18.36 +34:32:53.4 -- not an asteroid (will add it to exclusion list)
14:38:02.79 +34:17:52.0 -- not an asteroid (will add it to exclusion list)
14:46:18.89 +34:17:09.6 -- not an asteroid (will add it to exclusion list)
14:31:07.69 +33:20:04.1 -- not an asteroid (will add it to exclusion list)
14:38:09.09 +32:47:43.7 -- not an asteroid (will add it to exclusion list)
14:39:23.91 +33:26:36.0 -- not an asteroid (will add it to exclusion list)
14:40:51.66 +32:44:59.7 -- not an asteroid (will add it to exclusion list)
14:39:49.42 +32:55:42.7 -- not an asteroid (will add it to exclusion list)
14:42:58.35 +34:28:17.5 -- not an asteroid (will add it to exclusion list)
14:42:35.46 +33:31:52.6 -- not an asteroid (will add it to exclusion list)
14:39:06.28 +33:18:57.0 -- not an asteroid (will add it to exclusion list)
14:40:19.70 +34:44:54.8 -- not an asteroid (will add it to exclusion list)
14:41:36.27 +34:01:24.2 -- not an asteroid (will add it to exclusion list)
14:44:36.44 +33:27:30.7 -- not an asteroid (will add it to exclusion list)
14:40:05.44 +33:03:53.4 -- not an asteroid (will add it to exclusion list)
14:44:06.07 +34:19:01.8 -- not an asteroid (will add it to exclusion list)
14:43:08.60 +34:13:57.0 -- not an asteroid (will add it to exclusion list)
14:43:43.22 +33:04:52.1 -- not an asteroid (will add it to exclusion list)
14:38:47.35 +33:50:08.0 -- not an asteroid (will add it to exclusion list)
14:39:29.80 +33:13:49.2 -- not an asteroid (will add it to exclusion list)
14:43:46.91 +33:42:17.2 -- not an asteroid (will add it to exclusion list)
14:31:43.91 +32:58:42.6 -- not an asteroid (will add it to exclusion list)
14:45:28.10 +33:49:23.4 -- not an asteroid (will add it to exclusion list)
14:46:41.03 +33:57:01.9 -- not an asteroid (will add it to exclusion list)
14:38:37.97 +33:10:01.8 -- not an asteroid (will add it to exclusion list)
14:42:12.27 +34:00:50.5 -- not an asteroid (will add it to exclusion list)
14:44:37.70 +33:13:08.2 -- not an asteroid (will add it to exclusion list)
14:38:38.21 +34:56:25.9 -- not an asteroid (will add it to exclusion list)
14:44:38.13 +34:39:34.9 -- not an asteroid (will add it to exclusion list)
14:40:21.50 +32:42:29.1 -- not an asteroid (will add it to exclusion list)
14:40:14.26 +33:07:35.3 -- not an asteroid (will add it to exclusion list)
14:43:54.02 +32:49:21.7 -- not an asteroid (will add it to exclusion list)
14:38:56.04 +32:46:01.1 -- not an asteroid (will add it to exclusion list)
14:45:40.12 +34:06:19.0 -- not an asteroid (will add it to exclusion list)
14:40:00.82 +32:59:49.8 -- not an asteroid (will add it to exclusion list)
14:45:19.07 +33:50:39.5 -- not an asteroid (will add it to exclusion list)
14:44:25.67 +33:04:03.3 -- not an asteroid (will add it to exclusion list)
14:45:20.67 +33:35:20.7 -- not an asteroid (will add it to exclusion list)
14:42:27.30 +33:34:33.7 -- not an asteroid (will add it to exclusion list)
14:47:21.14 +35:19:44.3 -- not an asteroid (will add it to exclusion list)
14:41:14.37 +34:10:10.8 -- not an asteroid (will add it to exclusion list)
14:40:51.93 +33:37:42.1 -- not an asteroid (will add it to exclusion list)
14:46:18.85 +33:35:24.2 -- not an asteroid (will add it to exclusion list)
14:30:14.73 +33:08:23.9 -- not an asteroid (will add it to exclusion list)
14:39:05.73 +32:54:06.9 -- not an asteroid (will add it to exclusion list)
14:38:57.23 +33:54:23.5 -- not an asteroid (will add it to exclusion list)
14:40:31.57 +33:39:04.5 -- not an asteroid (will add it to exclusion list)
14:44:31.97 +35:36:12.3 -- not an asteroid (will add it to exclusion list)
14:47:03.20 +33:55:57.0 -- not an asteroid (will add it to exclusion list)
14:38:26.80 +32:48:05.0 -- not an asteroid (will add it to exclusion list)
14:40:20.22 +33:38:09.5 -- not an asteroid (will add it to exclusion list)
14:40:12.83 +32:50:49.8 -- not an asteroid (will add it to exclusion list)
14:44:00.28 +33:31:51.8 -- not an asteroid (will add it to exclusion list)
14:41:26.95 +32:54:47.6 -- not an asteroid (will add it to exclusion list)
14:45:54.62 +34:16:35.6 -- not an asteroid (will add it to exclusion list)
14:42:19.70 +33:49:51.2 -- not an asteroid (will add it to exclusion list)
14:42:09.13 +34:19:08.3 -- not an asteroid (will add it to exclusion list)
14:45:41.81 +33:16:28.0 -- not an asteroid (will add it to exclusion list)
14:30:15.10 +33:13:53.4 -- not an asteroid (will add it to exclusion list)
14:41:13.71 +32:52:10.4 -- not an asteroid (will add it to exclusion list)
14:43:53.18 +33:17:19.5 -- not an asteroid (will add it to exclusion list)
14:38:40.15 +33:25:18.8 -- not an asteroid (will add it to exclusion list)
14:45:59.09 +33:26:07.0 -- not an asteroid (will add it to exclusion list)
14:41:41.28 +33:16:00.6 -- not an asteroid (will add it to exclusion list)
14:46:47.00 +33:23:30.3 -- not an asteroid (will add it to exclusion list)
14:42:55.98 +32:56:36.8 -- not an asteroid (will add it to exclusion list)
14:43:39.43 +32:50:36.8 -- not an asteroid (will add it to exclusion list)
14:29:22.45 +32:57:09.8 -- not an asteroid (will add it to exclusion list)
14:48:21.86 +35:32:14.3 -- not an asteroid (will add it to exclusion list)
14:40:19.53 +33:50:46.4 -- not an asteroid (will add it to exclusion list)
14:42:30.21 +33:41:19.6 -- not an asteroid (will add it to exclusion list)
14:46:06.19 +34:11:31.7 -- not an asteroid (will add it to exclusion list)
14:47:24.88 +34:26:50.8 -- not an asteroid (will add it to exclusion list)
14:39:41.55 +33:18:44.0 -- not an asteroid (will add it to exclusion list)
14:47:19.41 +34:36:45.4 -- not an asteroid (will add it to exclusion list)
14:40:00.41 +32:52:38.2 -- not an asteroid (will add it to exclusion list)
14:30:35.86 +32:51:27.7 -- not an asteroid (will add it to exclusion list)
14:43:36.97 +33:24:51.0 -- not an asteroid (will add it to exclusion list)
14:40:13.55 +32:59:16.1 -- not an asteroid (will add it to exclusion list)
14:31:09.33 +33:26:17.8 -- not an asteroid (will add it to exclusion list)
14:46:35.14 +33:33:19.0 -- not an asteroid (will add it to exclusion list)
14:40:34.03 +33:03:30.4 -- not an asteroid (will add it to exclusion list)
14:42:56.40 +33:22:17.8 -- not an asteroid (will add it to exclusion list)
14:29:36.11 +33:15:57.6 -- not an asteroid (will add it to exclusion list)
14:44:05.31 +33:32:48.3 -- not an asteroid (will add it to exclusion list)
14:42:52.59 +33:30:38.0 -- not an asteroid (will add it to exclusion list)
14:41:33.81 +34:42:17.6 -- not an asteroid (will add it to exclusion list)
14:40:58.12 +33:16:33.8 -- not an asteroid (will add it to exclusion list)
14:43:59.90 +33:25:05.9 -- not an asteroid (will add it to exclusion list)
14:40:57.74 +32:44:27.4 -- not an asteroid (will add it to exclusion list)
14:31:44.70 +32:55:38.9 -- not an asteroid (will add it to exclusion list)
14:39:02.52 +33:25:56.4 -- not an asteroid (will add it to exclusion list)
14:31:27.70 +32:57:35.5 -- not an asteroid (will add it to exclusion list)
14:44:30.34 +33:10:00.4 -- not an asteroid (will add it to exclusion list)
14:42:58.89 +33:28:12.5 -- not an asteroid (will add it to exclusion list)
14:41:47.87 +33:25:58.9 -- not an asteroid (will add it to exclusion list)
14:41:49.41 +33:21:10.2 -- not an asteroid (will add it to exclusion list)
14:45:49.30 +33:34:58.9 -- not an asteroid (will add it to exclusion list)
14:44:58.15 +33:59:55.7 -- not an asteroid (will add it to exclusion list)
14:42:32.35 +33:37:47.2 -- not an asteroid (will add it to exclusion list)
14:42:06.38 +32:53:18.9 -- not an asteroid (will add it to exclusion list)
14:44:39.56 +33:44:37.7 -- not an asteroid (will add it to exclusion list)
14:40:03.76 +33:30:32.3 -- not an asteroid (will add it to exclusion list)
14:29:44.53 +32:56:51.9 -- not an asteroid (will add it to exclusion list)
14:37:53.69 +34:59:24.0 -- not an asteroid (will add it to exclusion list)
14:41:04.32 +32:43:16.8 -- not an asteroid (will add it to exclusion list)
14:41:48.74 +33:05:59.7 -- not an asteroid (will add it to exclusion list)
14:41:03.71 +33:44:36.0 -- not an asteroid (will add it to exclusion list)
14:43:12.48 +32:45:33.9 -- not an asteroid (will add it to exclusion list)
14:40:28.51 +32:57:54.7 -- not an asteroid (will add it to exclusion list)
14:43:45.04 +33:35:08.0 -- not an asteroid (will add it to exclusion list)
14:45:38.21 +34:40:36.0 -- not an asteroid (will add it to exclusion list)
14:40:20.88 +33:10:15.9 -- not an asteroid (will add it to exclusion list)
14:31:04.57 +32:57:28.1 -- not an asteroid (will add it to exclusion list)
14:43:23.54 +34:32:34.0 -- not an asteroid (will add it to exclusion list)
14:46:34.79 +34:16:12.8 -- not an asteroid (will add it to exclusion list)
14:47:00.58 +34:21:27.1 -- not an asteroid (will add it to exclusion list)
14:42:25.43 +33:16:10.6 -- not an asteroid (will add it to exclusion list)
14:45:39.19 +32:57:44.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
14:29:22.45 +32:57:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:29:36.11 +33:15:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:29:44.53 +32:56:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:30:14.73 +33:08:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:30:15.10 +33:13:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:30:35.86 +32:51:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:04.57 +32:57:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:07.69 +33:20:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:09.33 +33:26:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:27.70 +32:57:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:43.91 +32:58:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:31:44.70 +32:55:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:37:47.77 +34:53:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:37:53.69 +34:59:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:02.79 +34:17:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:09.09 +32:47:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:26.80 +32:48:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:36.92 +33:03:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:37.97 +33:10:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:38.21 +34:56:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:40.15 +33:25:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:41.93 +32:44:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:47.35 +33:50:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:56.04 +32:46:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:57.23 +33:54:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:38:58.30 +32:58:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:02.52 +33:25:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:05.73 +32:54:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:06.28 +33:18:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:23.91 +33:26:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:29.80 +33:13:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:41.55 +33:18:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:49.42 +32:55:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:00.41 +32:52:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:00.82 +32:59:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:03.76 +33:30:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:05.44 +33:03:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:08.44 +34:03:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:12.83 +32:50:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:13.55 +32:59:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:14.26 +33:07:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:19.53 +33:50:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:19.70 +34:44:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:20.22 +33:38:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:20.88 +33:10:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:21.50 +32:42:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:22.54 +33:36:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:28.51 +32:57:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:31.57 +33:39:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:34.03 +33:03:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:51.66 +32:44:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:51.93 +33:37:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:57.74 +32:44:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:40:58.12 +33:16:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:03.71 +33:44:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:04.32 +32:43:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:13.71 +32:52:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:14.37 +34:10:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:26.95 +32:54:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:33.81 +34:42:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:36.27 +34:01:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:41.28 +33:16:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:47.87 +33:25:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:48.74 +33:05:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:49.41 +33:21:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:51.32 +34:17:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:06.38 +32:53:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:09.13 +34:19:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:12.27 +34:00:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:19.70 +33:49:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:25.43 +33:16:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:27.30 +33:34:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:30.21 +33:41:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:32.35 +33:37:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:35.46 +33:31:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:52.59 +33:30:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:55.98 +32:56:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:56.40 +33:22:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:58.35 +34:28:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:58.89 +33:28:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:08.60 +34:13:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:12.48 +32:45:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:23.54 +34:32:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:36.97 +33:24:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:39.43 +32:50:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:43.22 +33:04:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:45.04 +33:35:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:46.91 +33:42:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:53.18 +33:17:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:54.02 +32:49:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:59.90 +33:25:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:00.28 +33:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:05.31 +33:32:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:06.07 +34:19:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:25.67 +33:04:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:30.34 +33:10:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:31.97 +35:36:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:36.44 +33:27:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:37.70 +33:13:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:38.13 +34:39:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:39.56 +33:44:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:58.15 +33:59:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:19.07 +33:50:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:20.67 +33:35:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:28.10 +33:49:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:38.21 +34:40:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:39.19 +32:57:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:40.12 +34:06:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:41.56 +33:56:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:41.81 +33:16:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:49.30 +33:34:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:54.62 +34:16:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:59.09 +33:26:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:06.19 +34:11:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:18.36 +34:32:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:18.85 +33:35:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:18.89 +34:17:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:34.79 +34:16:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:35.14 +33:33:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:41.03 +33:57:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:47.00 +33:23:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:00.58 +34:21:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:03.20 +33:55:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:05.29 +33:40:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:19.41 +34:36:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:21.14 +35:19:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:24.88 +34:26:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:32.83 +35:00:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:48:21.86 +35:32:14.3 -- 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)
14:29:22.45 +32:57:09.8 -- not a known variable star
14:29:36.11 +33:15:57.6 -- not a known variable star
14:29:44.53 +32:56:51.9 -- not a known variable star
14:30:14.73 +33:08:23.9 -- not a known variable star
14:30:15.10 +33:13:53.4 -- not a known variable star
14:30:35.86 +32:51:27.7 -- not a known variable star
14:31:04.57 +32:57:28.1 -- not a known variable star
14:31:07.69 +33:20:04.1 -- not a known variable star
14:31:09.33 +33:26:17.8 -- not a known variable star
14:31:27.70 +32:57:35.5 -- not a known variable star
14:31:43.91 +32:58:42.6 -- a known variable star
14:31:44.70 +32:55:38.9 -- not a known variable star
14:37:47.77 +34:53:56.4 -- not a known variable star
14:37:53.69 +34:59:24.0 -- a known variable star
14:38:02.79 +34:17:52.0 -- not a known variable star
14:38:09.09 +32:47:43.7 -- not a known variable star
14:38:26.80 +32:48:05.0 -- not a known variable star
14:38:36.92 +33:03:40.9 -- not a known variable star
14:38:37.97 +33:10:01.8 -- not a known variable star
14:38:38.21 +34:56:25.9 -- a known variable star
14:38:40.15 +33:25:18.8 -- not a known variable star
14:38:41.93 +32:44:48.0 -- not a known variable star
14:38:47.35 +33:50:08.0 -- not a known variable star
14:38:56.04 +32:46:01.1 -- not a known variable star
14:38:57.23 +33:54:23.5 -- not a known variable star
14:38:58.30 +32:58:24.2 -- not a known variable star
14:39:02.52 +33:25:56.4 -- not a known variable star
14:39:05.73 +32:54:06.9 -- not a known variable star
14:39:06.28 +33:18:57.0 -- a known variable star
14:39:23.91 +33:26:36.0 -- not a known variable star
14:39:29.80 +33:13:49.2 -- not a known variable star
14:39:41.55 +33:18:44.0 -- not a known variable star
14:39:49.42 +32:55:42.7 -- not a known variable star
14:40:00.41 +32:52:38.2 -- a known variable star
14:40:00.82 +32:59:49.8 -- not a known variable star
14:40:03.76 +33:30:32.3 -- not a known variable star
14:40:05.44 +33:03:53.4 -- not a known variable star
14:40:08.44 +34:03:57.7 -- a known variable star
14:40:12.83 +32:50:49.8 -- not a known variable star
14:40:13.55 +32:59:16.1 -- not a known variable star
14:40:14.26 +33:07:35.3 -- not a known variable star
14:40:19.53 +33:50:46.4 -- not a known variable star
14:40:19.70 +34:44:54.8 -- not a known variable star
14:40:20.22 +33:38:09.5 -- not a known variable star
14:40:20.88 +33:10:15.9 -- not a known variable star
14:40:21.50 +32:42:29.1 -- not a known variable star
14:40:22.54 +33:36:18.1 -- a known variable star
14:40:28.51 +32:57:54.7 -- not a known variable star
14:40:31.57 +33:39:04.5 -- not a known variable star
14:40:34.03 +33:03:30.4 -- not a known variable star
14:40:51.66 +32:44:59.7 -- not a known variable star
14:40:51.93 +33:37:42.1 -- not a known variable star
14:40:57.74 +32:44:27.4 -- not a known variable star
14:40:58.12 +33:16:33.8 -- a known variable star
14:41:03.71 +33:44:36.0 -- not a known variable star
14:41:04.32 +32:43:16.8 -- not a known variable star
14:41:13.71 +32:52:10.4 -- not a known variable star
14:41:14.37 +34:10:10.8 -- not a known variable star
14:41:26.95 +32:54:47.6 -- not a known variable star
14:41:33.81 +34:42:17.6 -- not a known variable star
14:41:36.27 +34:01:24.2 -- not a known variable star
14:41:41.28 +33:16:00.6 -- not a known variable star
14:41:47.87 +33:25:58.9 -- not a known variable star
14:41:48.74 +33:05:59.7 -- not a known variable star
14:41:49.41 +33:21:10.2 -- not a known variable star
14:41:51.32 +34:17:46.9 -- not a known variable star
14:42:06.38 +32:53:18.9 -- not a known variable star
14:42:09.13 +34:19:08.3 -- not a known variable star
14:42:12.27 +34:00:50.5 -- not a known variable star
14:42:19.70 +33:49:51.2 -- a known variable star
14:42:25.43 +33:16:10.6 -- not a known variable star
14:42:27.30 +33:34:33.7 -- not a known variable star
14:42:30.21 +33:41:19.6 -- not a known variable star
14:42:32.35 +33:37:47.2 -- a known variable star
14:42:35.46 +33:31:52.6 -- not a known variable star
14:42:52.59 +33:30:38.0 -- a known variable star
14:42:55.98 +32:56:36.8 -- not a known variable star
14:42:56.40 +33:22:17.8 -- not a known variable star
14:42:58.35 +34:28:17.5 -- not a known variable star
14:42:58.89 +33:28:12.5 -- not a known variable star
14:43:08.60 +34:13:57.0 -- not a known variable star
14:43:12.48 +32:45:33.9 -- not a known variable star
14:43:23.54 +34:32:34.0 -- not a known variable star
14:43:36.97 +33:24:51.0 -- not a known variable star
14:43:39.43 +32:50:36.8 -- not a known variable star
14:43:43.22 +33:04:52.1 -- not a known variable star
14:43:45.04 +33:35:08.0 -- not a known variable star
14:43:46.91 +33:42:17.2 -- not a known variable star
14:43:53.18 +33:17:19.5 -- not a known variable star
14:43:54.02 +32:49:21.7 -- not a known variable star
14:43:59.90 +33:25:05.9 -- not a known variable star
14:44:00.28 +33:31:51.8 -- not a known variable star
14:44:05.31 +33:32:48.3 -- not a known variable star
14:44:06.07 +34:19:01.8 -- not a known variable star
14:44:25.67 +33:04:03.3 -- not a known variable star
14:44:30.34 +33:10:00.4 -- not a known variable star
14:44:31.97 +35:36:12.3 -- not a known variable star
14:44:36.44 +33:27:30.7 -- not a known variable star
14:44:37.70 +33:13:08.2 -- not a known variable star
14:44:38.13 +34:39:34.9 -- not a known variable star
14:44:39.56 +33:44:37.7 -- not a known variable star
14:44:58.15 +33:59:55.7 -- not a known variable star
14:45:19.07 +33:50:39.5 -- not a known variable star
14:45:20.67 +33:35:20.7 -- not a known variable star
14:45:28.10 +33:49:23.4 -- not a known variable star
14:45:38.21 +34:40:36.0 -- not a known variable star
14:45:39.19 +32:57:44.3 -- not a known variable star
14:45:40.12 +34:06:19.0 -- not a known variable star
14:45:41.56 +33:56:14.9 -- not a known variable star
14:45:41.81 +33:16:28.0 -- a known variable star
14:45:49.30 +33:34:58.9 -- not a known variable star
14:45:54.62 +34:16:35.6 -- not a known variable star
14:45:59.09 +33:26:07.0 -- not a known variable star
14:46:06.19 +34:11:31.7 -- not a known variable star
14:46:18.36 +34:32:53.4 -- not a known variable star
14:46:18.85 +33:35:24.2 -- a known variable star
14:46:18.89 +34:17:09.6 -- not a known variable star
14:46:34.79 +34:16:12.8 -- not a known variable star
14:46:35.14 +33:33:19.0 -- not a known variable star
14:46:41.03 +33:57:01.9 -- a known variable star
14:46:47.00 +33:23:30.3 -- not a known variable star
14:47:00.58 +34:21:27.1 -- not a known variable star
14:47:03.20 +33:55:57.0 -- not a known variable star
14:47:05.29 +33:40:44.3 -- not a known variable star
14:47:19.41 +34:36:45.4 -- not a known variable star
14:47:21.14 +35:19:44.3 -- not a known variable star
14:47:24.88 +34:26:50.8 -- a known variable star
14:47:32.83 +35:00:24.8 -- not a known variable star
14:48:21.86 +35:32:14.3 -- not a known variable star
Found 114 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
129 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 129 (excluding asteroids and hot pixels, 114 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)2461206.66548191 -observatory V36
07:19:30.52 +23:18:13.8 Mercury (0.5mag)
08:17:24.71 +21:46:36.1 Venus (-4.0mag)
03:09:55.90 +17:13:12.3 Mars (1.3mag)
07:54:19.81 +21:16:15.6 Jupiter (-1.8mag)
00:51:14.67 +02:58:42.5 Saturn (0.8mag)
04:01:50.75 +20:30:08.6 Uranus (5.8mag)
00:16:30.33 +00:18:46.4 Neptune (7.8mag)
20:32:56.08 -23:07:14.9 Pluto (14.5mag)
05:31:47.62 +27:12:02.9 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Jun 14 23:30 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461206.66548191:
07:54:18.42 +21:16:21.9 Io (6.2mag)
07:54:17.62 +21:16:24.5 Europa (6.3mag)
07:54:04.78 +21:17:01.8 Ganymede (5.6mag)
07:53:54.24 +21:17:37.4 Callisto (6.9mag)
07:54:12.20 +20:53:18.2 Himalia (15.6mag)
07:54:19.53 +21:16:16.6 Thebe (16.5mag)
07:54:00.06 +21:05:46.4 Elara (17.6mag)
07:56:51.38 +21:24:08.8 Pasiphae (17.8mag)
08:00:35.96 +21:18:31.5 Carme (18.9mag)
00:51:26.70 +02:58:40.3 Titan (8.6mag)
00:51:19.58 +02:58:35.8 Rhea (9.9mag)
00:51:39.14 +03:01:15.1 Iapetus (11.3mag)
00:51:30.05 +02:58:31.6 Hyperion (14.6mag)
00:51:48.28 +02:59:38.3 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 14 23:30 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461206.66548191:
17:28:24.93 -35:35:57.2 JWST
18:55:55.05 +19:43:36.3 Chandra
08:23:45.60 -45:43:35.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 14 23:30 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461206.66548191 -observatory V36
18:38:25.31 -33:08:25.9 13.6mag P/2010 H2 (Vales)
06:00:22.72 -68:00:35.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:51:38.26 +32:03:41.4 17.5mag C/2017 K2 (PANSTARRS)
17:11:56.98 +15:39:28.8 17.8mag C/2021 G2 (ATLAS)
22:20:28.16 -43:49:59.8 16.3mag P/2021 N1 (ZTF)
23:10:49.39 +31:50:23.0 17.2mag C/2022 E2 (ATLAS)
05:42:33.64 +27:00:18.7 16.5mag C/2022 N2 (PANSTARRS)
09:34:52.90 +30:49:45.9 16.7mag C/2022 QE78 (ATLAS)
08:54:23.26 +04:14:35.3 17.7mag C/2022 R6 (PANSTARRS)
18:23:37.67 +21:41:35.4 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:17:00.89 -11:02:00.3 17.6mag P/2023 B1 (PANSTARRS)
22:11:26.97 +66:55:40.2 17.8mag C/2023 H5 (Lemmon)
17:29:02.34 -07:23:31.0 13.7mag C/2023 R1 (PANSTARRS)
13:16:36.80 +81:22:36.4 18.0mag C/2023 X2 (Lemmon)
07:20:21.84 +64:33:28.9 17.7mag C/2024 A1 (ATLAS)
06:57:42.37 +28:25:09.4 13.9mag C/2024 E1 (Wierzchos)
15:31:58.48 +14:05:17.2 17.4mag C/2024 G6 (ATLAS)
20:07:55.57 +33:10:19.7 13.9mag C/2024 J3 (ATLAS)
04:25:00.49 -15:22:10.2 16.0mag C/2024 T5 (ATLAS)
06:12:22.64 +33:17:26.7 17.9mag C/2025 J1 (Borisov)
11:32:34.60 +52:19:52.8 17.7mag C/2025 L1 (ATLAS)
06:52:49.46 -11:11:56.9 14.7mag C/2025 R3 (PANSTARRS)
09:30:08.42 +23:13:32.2 17.9mag C/2025 V2 (Rankin)
12:39:47.55 +04:38:12.4 17.1mag C/2025 Y1 (ATLAS)
18:00:08.33 +76:31:24.5 17.8mag C/2026 A2 (Bok)
02:12:20.57 +43:53:19.4 16.2mag C/2026 B2 (Sun-Gao)
11:13:08.93 -01:26:12.5 16.6mag A/2026 E1
20:36:13.25 -09:13:36.8 8.4mag 10P/Tempel
11:03:49.91 -01:05:20.5 16.0mag 29P/Schwassmann-Wachmann
03:22:28.49 +26:33:39.4 17.7mag 47P/Ashbrook-Jackson
09:14:50.81 +21:44:56.2 16.9mag 63P/Wild
00:32:39.97 -05:57:09.1 15.6mag 65P/Gunn
07:06:05.65 +34:00:53.5 17.1mag 76P/West-Kohoutek-Ikemura
03:26:04.84 +18:03:29.3 13.8mag 78P/Gehrels
01:35:32.84 +06:18:39.2 15.7mag 88P/Howell
05:17:03.42 +30:43:25.7 15.3mag 93P/Lovas
03:03:01.06 +28:40:52.7 17.4mag 114P/Wiseman-Skiff
07:07:16.48 +32:43:59.1 15.5mag 123P/West-Hartley
10:02:24.23 +11:39:55.9 16.6mag 124P/Mrkos
04:10:32.57 +19:41:26.4 16.3mag 128P/Shoemaker-Holt
04:47:23.80 +19:21:55.9 17.8mag 131P/Mueller
06:27:13.86 +17:45:00.9 15.5mag 141P/Machholz
06:30:19.67 +17:53:34.4 15.5mag 141P-A/Machholz
05:28:28.04 +16:56:53.6 12.4mag 141P-D/Machholz
03:02:29.21 -23:46:18.2 16.6mag 161P/Hartley-IRAS
04:04:45.80 +26:29:32.2 15.0mag 162P/SidingSpring
19:35:08.39 +03:54:30.1 16.5mag 169P/NEAT
00:36:59.27 +03:47:20.5 17.8mag 220P/McNaught
16:47:05.23 -08:12:21.1 16.5mag 235P/LINEAR
07:50:21.06 +35:09:31.4 17.6mag 240P/NEAT
00:50:44.73 +00:32:44.1 16.2mag 260P/McNaught
04:23:27.26 +33:41:18.5 17.5mag 295P/LINEAR
00:31:42.84 -01:36:31.8 17.8mag 320P/McNaught
15:12:19.81 +07:48:46.6 17.5mag 391P/Kowalski
08:12:47.47 +20:33:21.8 17.9mag 450P/LONEOS
07:11:20.15 +41:11:31.4 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 14 23:30 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
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
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:26:28.11 -72:31:19.50 2026-06-11 17.05
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:26:28.11 -72:31:19.50 2026-06-11 17.05
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
-rw-r--r-- 1 apache apache 5.6K Jun 14 23:30 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
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
-rw-r--r-- 1 apache apache 189K Jun 14 23:30 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:49:19.289 -10:17:13.45 AT 2026ome 2026-06-06.42 19.9
15:05:48.011 -29:45:37.21 AT 2026omd 2026-06-06.50 20.04
20:30:10.926 -29:56:07.53 AT 2026omc 2026-06-07.64 18.81
19:50:57.124 -53:24:23.12 AT 2026omb 2026-06-06.67 20.17
23:28:37.442 -43:16:54.75 AT 2026oma 2026-06-06.73 19.64
11:48:30.394 -39:49:36.11 AT 2026olz 2026-06-06.77 19.237
13:56:31.281 +70:50:34.89 AT 2026oly 2026-06-06.35 19.395
12:22:49.169 -21:19:33.91 AT 2026olx 2026-06-07.30 18.696
22:49:46.803 -26:24:12.60 SN 2026olw 2026-06-07.58 18.251
10:47:10.687 -70:44:55.20 AT 2026olv 2026-06-06.81 18.37
11:06:55.086 +37:19:50.72 AT 2026olu 2026-06-01.30 18.692
14:54:40.331 -10:41:24.18 SN 2026olt 2026-06-04.43 18.588
10:58:43.462 +36:47:26.62 AT 2026ols 2026-06-04.90 18.501
08:45:48.069 -64:46:34.13 AT 2026olr 2026-06-06.71 18.616
10:02:19.987 -84:42:35.43 AT 2026olq 2026-06-06.80 18.714
22:35:38.444 -55:59:06.00 SN 2026olp 2026-05-30.09 18.424
21:02:06.402 +85:28:22.07 AT 2026olo 2026-06-07.10 18.987
18:52:00.191 +72:19:28.04 AT 2026oln 2026-06-07.07 18.528
23:35:46.181 -42:09:54.16 AT 2026olm 2026-06-07.13 18.697
12:34:21.767 -10:29:46.08 AT 2026oll 2026-06-05.82 19.393
-rw-r--r-- 1 apache apache 30K Jun 14 23:30 tns_transients_list.txt
