This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH
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 07 16.2413 2461237.7413 13.19 14:47:14.57 +21:23:23.3
26.98773 63.05343 galactic Boo Second-epoch detections are separated by 0.5" and 5.1 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 | 14:47:14.57 +21:23:23.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.408+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:47:14.57 +21:23:23.3: 14.06 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:47:14.57 +21:23:23.3: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461237.7413,13.19,0.05,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 20260716.2413 13.19CV 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 07 16.2413 2461237.7413 13.41 14:50:47.14 +22:04:01.8
28.93683 62.47025 galactic Boo Second-epoch detections are separated by 1.5" and 5.2 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 | 14:50:47.14 +22:04:01.8 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.033 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:47.14 +22:04:01.8: 14.35 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:47.14 +22:04:01.8: 14.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.46 14:52:32.93 +20:57:07.9
26.93098 61.74160 galactic Boo Second-epoch detections are separated by 1.4" and 5.0 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 | 14:52:32.93 +20:57:07.9 (user input) | T | P | (position from user input) J-Ks=0.636+/-0.029 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:52:32.93 +20:57:07.9: 14.38 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:52:32.93 +20:57:07.9: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461237.7413,13.46,0.05,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 20260716.2413 13.46CV 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 07 16.2413 2461237.7413 13.34 14:42:31.77 +22:13:00.0
28.03092 64.34458 galactic Boo Second-epoch detections are separated by 1.5" and 5.3 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 | 14:42:31.77 +22:13:00.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.440+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:42:31.77 +22:13:00.0: 14.43 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:42:31.77 +22:13:00.0: 14.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461237.7413,13.34,0.05,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 20260716.2413 13.34CV 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 07 16.2413 2461237.7413 13.55 14:51:02.72 +20:09:49.6
25.11137 61.81269 galactic Boo Second-epoch detections are separated by 1.0" and 5.1 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 | 14:51:02.72 +20:09:49.6 (user input) | T | P | (position from user input) J-Ks=0.671+/-0.032 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:51:02.72 +20:09:49.6: 14.55 +/- 0.08 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:51:02.72 +20:09:49.6: 14.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.59 +/- 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,2461237.7413,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.55CV 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 07 16.2413 2461237.7413 12.92 14:48:41.41 +21:56:23.9
28.36524 62.89839 galactic Boo Second-epoch detections are separated by 0.8" and 5.1 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 | 14:48:41.41 +21:56:23.9 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.036 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:48:41.41 +21:56:23.9: 13.79 +/- 0.04 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:48:41.41 +21:56:23.9: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461237.7413,12.92,0.05,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 20260716.2413 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 07 16.2413 2461237.7413 13.07 14:47:16.18 +19:52:46.5
23.87680 62.54437 galactic Boo Second-epoch detections are separated by 0.4" and 5.1 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 | 14:47:16.18 +19:52:46.5 (user input) | T | P | (position from user input) J-Ks=0.607+/-0.028 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:47:16.18 +19:52:46.5: 13.96 +/- 0.04 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:47:16.18 +19:52:46.5: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461237.7413,13.07,0.05,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 20260716.2413 13.07CV 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 07 16.2413 2461237.7413 13.05 14:52:19.68 +20:11:48.3
25.39365 61.54113 galactic Boo Second-epoch detections are separated by 0.9" and 5.1 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 | 14:52:19.68 +20:11:48.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.508+/-0.029 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:52:19.68 +20:11:48.3: 13.99 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:52:19.68 +20:11:48.3: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461237.7413,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.43 14:49:02.91 +21:51:46.6
28.25723 62.79634 galactic Boo Second-epoch detections are separated by 1.7" and 5.3 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 | 14:49:02.91 +21:51:46.6 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.036 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:02.91 +21:51:46.6: 14.47 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:02.91 +21:51:46.6: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461237.7413,13.43,0.05,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 20260716.2413 13.43CV 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 07 16.2413 2461237.7413 13.44 14:46:04.65 +20:54:15.4
25.77904 63.15652 galactic Boo Second-epoch detections are separated by 2.2" and 5.0 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 | 14:46:04.65 +20:54:15.4 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.038 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:46:04.65 +20:54:15.4: 14.46 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:46:04.65 +20:54:15.4: 14.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.46 +/- 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,2461237.7413,13.44,0.05,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 20260716.2413 13.44CV 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 07 16.2413 2461237.7413 13.21 14:56:05.44 +18:33:59.2
22.93140 60.12473 galactic Boo Second-epoch detections are separated by 0.9" and 5.0 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 | 14:56:05.44 +18:33:59.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.459+/-0.036 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:56:05.44 +18:33:59.2: 14.14 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:56:05.44 +18:33:59.2: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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,2461237.7413,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.38 15:01:42.52 +17:30:57.6
22.05878 58.48507 galactic Boo Second-epoch detections are separated by 1.1" and 5.3 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 | 15:01:42.52 +17:30:57.6 (user input) | T | P | (position from user input) J-Ks=0.154+/-0.041 (F)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 15:01:42.52 +17:30:57.6: 14.26 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 15:01:42.52 +17:30:57.6: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461237.7413,13.38,0.05,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 20260716.2413 13.38CV 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 07 16.2413 2461237.7413 13.34 14:50:56.45 +21:25:35.0
27.64076 62.24586 galactic Boo Second-epoch detections are separated by 0.6" and 5.1 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 | 14:50:56.45 +21:25:35.0 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.030 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:56.45 +21:25:35.0: 14.30 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:56.45 +21:25:35.0: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461237.7413,13.34,0.05,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 20260716.2413 13.34CV 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 07 16.2413 2461237.7413 13.38 15:09:14.81 +23:55:35.6
34.84323 58.84251 galactic Boo Second-epoch detections are separated by 2.1" and 5.2 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 | 15:09:14.81 +23:55:35.6 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.409+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 15:09:14.81 +23:55:35.6: 14.31 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 15:09:14.81 +23:55:35.6: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461237.7413,13.38,0.05,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 20260716.2413 13.38CV 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 07 16.2413 2461237.7413 13.19 14:44:44.70 +19:38:15.1
22.91461 63.01097 galactic Boo Second-epoch detections are separated by 1.1" and 5.3 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 | 14:44:44.70 +19:38:15.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.449+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:44:44.70 +19:38:15.1: 14.15 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:44:44.70 +19:38:15.1: 14.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 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,2461237.7413,13.19,0.05,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 20260716.2413 13.19CV 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 07 16.2413 2461237.7413 13.40 14:53:03.91 +18:51:25.7
22.92622 60.89786 galactic Boo Second-epoch detections are separated by 1.0" and 5.0 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 | 14:53:03.91 +18:51:25.7 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.032 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:53:03.91 +18:51:25.7: 14.33 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:53:03.91 +18:51:25.7: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461237.7413,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.05 14:46:35.12 +19:48:28.9
23.60660 62.66912 galactic Boo Second-epoch detections are separated by 1.8" and 4.8 pix
The object was found in VSX 1" CSS_J144635.1+194829
Type: EW
# Max. Min./Amp. JD0 Period
14.139 g Y 0.262 g 2458606.93920 0.284247000000
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:46:35.12 +19:48:28.9: 14.04 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:46:35.12 +19:48:28.9: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.97 +/- 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_J144635.1+194829,2461237.7413,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J144635.1+194829 20260716.2413 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.21 14:49:19.28 +21:12:48.4
26.95160 62.53845 galactic Boo Second-epoch detections are separated by 0.6" and 5.1 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 | 14:49:19.28 +21:12:48.4 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.391+/-0.038 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:19.28 +21:12:48.4: 14.18 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:19.28 +21:12:48.4: 14.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.20 +/- 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,2461237.7413,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.39 14:52:10.85 +20:51:22.9
26.68086 61.79230 galactic Boo Second-epoch detections are separated by 1.2" and 4.9 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 | 14:52:10.85 +20:51:22.9 (user input) | T | P | (position from user input) J-Ks=0.738+/-0.032 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:52:10.85 +20:51:22.9: 14.19 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:52:10.85 +20:51:22.9: 14.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461237.7413,13.39,0.05,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 20260716.2413 13.39CV 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 07 16.2413 2461237.7413 13.45 14:49:54.86 +21:19:37.0
27.27835 62.44258 galactic Boo Second-epoch detections are separated by 0.7" and 4.9 pix
The object was found in VSX 1" Gaia DR3 1238404277354577792
Type: ROT
# Max. Min./Amp. JD0 Period
13.980 G 14.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:54.86 +21:19:37.0: 14.36 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:54.86 +21:19:37.0: 14.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.43 +/- 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
Gaia DR3 1238404277354577792,2461237.7413,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1238404277354577792 20260716.2413 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.52 14:49:13.13 +22:22:29.6
29.35701 62.90501 galactic Boo Second-epoch detections are separated by 0.8" and 5.0 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 | 14:49:13.13 +22:22:29.6 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:13.13 +22:22:29.6: 14.35 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:13.13 +22:22:29.6: 14.57 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 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,2461237.7413,13.52,0.05,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 20260716.2413 13.52CV 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 07 16.2413 2461237.7413 13.62 14:47:51.84 +20:17:40.5
24.82616 62.55856 galactic Boo Second-epoch detections are separated by 1.3" and 4.9 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 | 14:47:51.84 +20:17:40.5 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:47:51.84 +20:17:40.5: 14.87 +/- 0.10 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:47:51.84 +20:17:40.5: 14.78 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.7413,13.62,0.05,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 20260716.2413 13.62CV 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 07 16.2413 2461237.7413 13.38 14:45:29.22 +21:21:01.6
26.62180 63.42960 galactic Boo Second-epoch detections are separated by 2.0" and 5.0 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 | 14:45:29.22 +21:21:01.6 (user input) | T | P | (position from user input) J-Ks=0.503+/-0.033 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:45:29.22 +21:21:01.6: 14.33 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:45:29.22 +21:21:01.6: 14.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.33 +/- 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,2461237.7413,13.38,0.05,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 20260716.2413 13.38CV 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 07 16.2413 2461237.7413 13.32 14:41:35.97 +22:39:11.3
28.86452 64.67320 galactic Boo Second-epoch detections are separated by 0.7" and 5.1 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 | 14:41:35.97 +22:39:11.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.525+/-0.034 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:41:35.97 +22:39:11.3: 14.19 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:41:35.97 +22:39:11.3: 14.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461237.7413,13.32,0.05,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 20260716.2413 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.29 14:44:00.95 +21:57:50.3
27.70623 63.94165 galactic Boo Second-epoch detections are separated by 1.6" and 5.3 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 | 14:44:00.95 +21:57:50.3 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.556+/-0.030 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:44:00.95 +21:57:50.3: 14.19 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:44:00.95 +21:57:50.3: 14.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461237.7413,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.26 14:59:47.41 +18:43:41.3
23.88400 59.37386 galactic Boo Second-epoch detections are separated by 0.9" and 4.9 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 | 14:59:47.41 +18:43:41.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.346+/-0.031 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:59:47.41 +18:43:41.3: 14.19 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:59:47.41 +18:43:41.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461237.7413,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.27 14:55:48.70 +19:05:34.4
23.86555 60.38298 galactic Boo Second-epoch detections are separated by 2.4" 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 | 14:55:48.70 +19:05:34.4 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.029 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:55:48.70 +19:05:34.4: 14.19 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:55:48.70 +19:05:34.4: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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,2461237.7413,13.27,0.05,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 20260716.2413 13.27CV 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 07 16.2413 2461237.7413 13.21 14:49:19.25 +21:07:14.4
26.76069 62.50931 galactic Boo Second-epoch detections are separated by 0.6" and 5.1 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 | 14:49:19.25 +21:07:14.4 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:19.25 +21:07:14.4: 14.16 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:19.25 +21:07:14.4: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461237.7413,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.38 14:52:23.49 +20:17:33.7
25.59371 61.55970 galactic Boo Second-epoch detections are separated by 0.7" and 5.1 pix
The object was found in VSX 0" Gaia DR3 1237326000045072768
Type: ROT
# Max. Min./Amp. JD0 Period
14.170 G 14.220 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:52:23.49 +20:17:33.7: 14.49 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:52:23.49 +20:17:33.7: 14.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.49 +/- 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
Gaia DR3 1237326000045072768,2461237.7413,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1237326000045072768 20260716.2413 13.38CV 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 07 16.2413 2461237.7413 13.66 14:49:50.37 +21:24:43.8
27.44206 62.48546 galactic Boo Second-epoch detections are separated by 1.1" 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 | 14:49:50.37 +21:24:43.8 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.042 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:50.37 +21:24:43.8: 14.69 +/- 0.08 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:50.37 +21:24:43.8: 14.89 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.77 +/- 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,2461237.7413,13.66,0.05,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 20260716.2413 13.66CV 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 07 16.2413 2461237.7413 13.11 14:42:27.08 +22:09:23.1
27.88562 64.34453 galactic Boo Second-epoch detections are separated by 0.9" and 5.1 pix
The object was found in VSX 1" Gaia DR3 1241638765685930880
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:42:27.08 +22:09:23.1: 14.06 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:42:27.08 +22:09:23.1: 14.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 1241638765685930880,2461237.7413,13.11,0.05,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 1241638765685930880 20260716.2413 13.11CV 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 07 16.2413 2461237.7413 13.53 14:47:39.32 +21:24:53.4
27.10567 62.96988 galactic Boo Second-epoch detections are separated by 0.5" and 5.1 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 | 14:47:39.32 +21:24:53.4 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.030 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:47:39.32 +21:24:53.4: 14.47 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:47:39.32 +21:24:53.4: 14.49 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.48 +/- 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,2461237.7413,13.53,0.05,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
target 20260716.2413 13.53CV 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 07 16.2413 2461237.7413 13.32 14:50:05.56 +21:03:33.4
26.75829 62.31910 galactic Boo Second-epoch detections are separated by 0.9" and 5.1 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 | 14:50:05.56 +21:03:33.4 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.036 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:05.56 +21:03:33.4: 14.31 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:05.56 +21:03:33.4: 14.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461237.7413,13.32,0.05,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 20260716.2413 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.04 14:49:48.08 +20:37:48.1
25.83784 62.24427 galactic Boo Second-epoch detections are separated by 1.2" and 5.3 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 | 14:49:48.08 +20:37:48.1 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:48.08 +20:37:48.1: 13.99 +/- 0.04 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:48.08 +20:37:48.1: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461237.7413,13.04,0.05,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 20260716.2413 13.04CV 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 07 16.2413 2461237.7413 13.53 14:55:39.73 +19:34:16.4
24.74513 60.58863 galactic Boo Second-epoch detections are separated by 1.5" 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 | 14:55:39.73 +19:34:16.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:55:39.73 +19:34:16.4: 14.62 +/- 0.09 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:55:39.73 +19:34:16.4: 14.72 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.7413,13.53,0.05,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
target 20260716.2413 13.53CV 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 07 16.2413 2461237.7413 13.41 14:51:13.22 +21:25:54.9
27.69474 62.18563 galactic Boo Second-epoch detections are separated by 1.6" and 5.0 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 | 14:51:13.22 +21:25:54.9 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.037 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:51:13.22 +21:25:54.9: 14.28 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:51:13.22 +21:25:54.9: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 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,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.48 14:50:19.32 +21:26:40.0
27.58288 62.38848 galactic Boo Second-epoch detections are separated by 2.5" and 5.2 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 | 14:50:19.32 +21:26:40.0 (user input) | T | P | (position from user input) J-Ks=0.565+/-0.036 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:19.32 +21:26:40.0: 14.46 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:19.32 +21:26:40.0: 14.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.50 +/- 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,2461237.7413,13.48,0.05,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 20260716.2413 13.48CV 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 07 16.2413 2461237.7413 13.23 14:50:00.88 +19:39:05.3
23.91483 61.85968 galactic Boo Second-epoch detections are separated by 0.8" and 5.2 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 | 14:50:00.88 +19:39:05.3 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:00.88 +19:39:05.3: 14.11 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:00.88 +19:39:05.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461237.7413,13.23,0.05,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 20260716.2413 13.23CV 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 07 16.2413 2461237.7413 13.18 14:56:24.00 +18:14:50.5
22.39841 59.93420 galactic Boo Second-epoch detections are separated by 2.0" and 5.0 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 | 14:56:24.00 +18:14:50.5 (user input) | T | P | (position from user input) J-Ks=0.531+/-0.035 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:56:24.00 +18:14:50.5: 14.12 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:56:24.00 +18:14:50.5: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461237.7413,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.10 14:58:27.85 +18:16:20.5
22.82033 59.49204 galactic Boo Second-epoch detections are separated by 0.5" and 5.1 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 | 14:58:27.85 +18:16:20.5 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.031 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:58:27.85 +18:16:20.5: 13.97 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:58:27.85 +18:16:20.5: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461237.7413,13.10,0.05,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 20260716.2413 13.10CV 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 07 16.2413 2461237.7413 13.22 14:46:44.84 +20:40:40.0
25.42099 62.93410 galactic Boo Second-epoch detections are separated by 0.4" and 5.1 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 | 14:46:44.84 +20:40:40.0 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.033 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:46:44.84 +20:40:40.0: 14.09 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:46:44.84 +20:40:40.0: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461237.7413,13.22,0.05,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 20260716.2413 13.22CV 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 07 16.2413 2461237.7413 13.41 14:42:25.67 +22:42:03.4
29.09289 64.50234 galactic Boo Second-epoch detections are separated by 0.9" and 5.2 pix
The object was found in VSX 2" Gaia DR3 1241812729041137536
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.770 G M
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:42:25.67 +22:42:03.4: 14.46 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:42:25.67 +22:42:03.4: 14.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.43 +/- 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
Gaia DR3 1241812729041137536,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1241812729041137536 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.49 14:48:49.66 +21:24:23.3
27.27276 62.70777 galactic Boo Second-epoch detections are separated by 1.3" and 5.2 pix
The object was found in VSX 0" Gaia DR3 1238454854889438080
Type: RS
# Max. Min./Amp. JD0 Period
14.190 G 14.280 G G
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:48:49.66 +21:24:23.3: 14.45 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:48:49.66 +21:24:23.3: 14.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.49 +/- 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
Gaia DR3 1238454854889438080,2461237.7413,13.49,0.05,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 1238454854889438080 20260716.2413 13.49CV 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 07 16.2413 2461237.7413 13.53 14:50:53.85 +19:22:50.6
23.54131 61.56770 galactic Boo Second-epoch detections are separated by 0.5" and 5.1 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 | 14:50:53.85 +19:22:50.6 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.033 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:53.85 +19:22:50.6: 14.61 +/- 0.08 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:53.85 +19:22:50.6: 14.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.57 +/- 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,2461237.7413,13.53,0.05,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
target 20260716.2413 13.53CV 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 07 16.2413 2461237.7413 13.46 14:54:04.15 +18:17:36.3
22.04980 60.46172 galactic Boo Second-epoch detections are separated by 0.9" and 5.0 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 | 14:54:04.15 +18:17:36.3 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:54:04.15 +18:17:36.3: 14.42 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:54:04.15 +18:17:36.3: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 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,2461237.7413,13.46,0.05,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 20260716.2413 13.46CV 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 07 16.2413 2461237.7413 13.43 14:56:04.45 +19:08:14.6
23.99526 60.34161 galactic Boo Second-epoch detections are separated by 1.2" and 5.0 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 | 14:56:04.45 +19:08:14.6 (user input) | T | P | (position from user input) J-Ks=0.725+/-0.029 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:56:04.45 +19:08:14.6: 14.42 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:56:04.45 +19:08:14.6: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 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,2461237.7413,13.43,0.05,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 20260716.2413 13.43CV 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 07 16.2413 2461237.7413 13.29 14:50:35.15 +19:25:52.2
23.58367 61.65453 galactic Boo Second-epoch detections are separated by 2.1" and 5.4 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 | 14:50:35.15 +19:25:52.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:35.15 +19:25:52.2: 14.42 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:35.15 +19:25:52.2: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461237.7413,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.35 14:53:43.40 +19:30:08.2
24.27916 60.99076 galactic Boo Second-epoch detections are separated by 1.3" and 5.0 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 | 14:53:43.40 +19:30:08.2 (user input) | T | P | (position from user input) J-Ks=0.765+/-0.030 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:53:43.40 +19:30:08.2: 14.41 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:53:43.40 +19:30:08.2: 14.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.44 +/- 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,2461237.7413,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.37 14:48:37.68 +19:39:49.9
23.68927 62.16876 galactic Boo Second-epoch detections are separated by 0.4" and 5.1 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 | 14:48:37.68 +19:39:49.9 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.037 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:48:37.68 +19:39:49.9: 14.26 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:48:37.68 +19:39:49.9: 14.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.29 +/- 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,2461237.7413,13.37,0.05,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 20260716.2413 13.37CV 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 07 16.2413 2461237.7413 13.41 15:07:31.46 +25:03:07.4
36.82359 59.46660 galactic Boo Second-epoch detections are separated by 0.8" and 4.8 pix
The object was found in VSX 1" HU Boo
Type: RRC
# Max. Min./Amp. JD0 Period
14.260 CV Y 0.490 CV 2451408.10200 0.337278000000
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 15:07:31.46 +25:03:07.4: 14.56 +/- 0.09 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 15:07:31.46 +25:03:07.4: 14.57 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.57 +/- 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
HU Boo,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HU Boo 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.25 14:47:24.46 +21:19:40.3
26.88426 62.99769 galactic Boo Second-epoch detections are separated by 0.5" and 5.1 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 | 14:47:24.46 +21:19:40.3 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:47:24.46 +21:19:40.3: 14.24 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:47:24.46 +21:19:40.3: 14.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461237.7413,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.53 14:56:11.12 +18:27:34.6
22.75061 60.06315 galactic Boo Second-epoch detections are separated by 2.3" and 5.2 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 | 14:56:11.12 +18:27:34.6 (user input) | T | P | (position from user input) J-Ks=0.668+/-0.034 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:56:11.12 +18:27:34.6: 14.64 +/- 0.09 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:56:11.12 +18:27:34.6: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.46 +/- 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,2461237.7413,13.53,0.05,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
target 20260716.2413 13.53CV 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 07 16.2413 2461237.7413 13.41 15:00:05.12 +18:35:27.5
23.68596 59.25772 galactic Boo Second-epoch detections are separated by 0.9" and 5.2 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 | 15:00:05.12 +18:35:27.5 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 15:00:05.12 +18:35:27.5: 14.38 +/- 0.08 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 15:00:05.12 +18:35:27.5: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.21 14:45:19.01 +21:35:50.1
27.12019 63.54354 galactic Boo Second-epoch detections are separated by 0.8" and 5.1 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 | 14:45:19.01 +21:35:50.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.391+/-0.033 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:45:19.01 +21:35:50.1: 14.08 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:45:19.01 +21:35:50.1: 14.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461237.7413,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.46 14:54:05.86 +20:50:48.9
26.96445 61.36520 galactic Boo Second-epoch detections are separated by 2.3" and 5.2 pix
The object was found in VSX 1" Gaia DR3 1262138335351551872
Type: ROT
# Max. Min./Amp. JD0 Period
13.990 G 14.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:54:05.86 +20:50:48.9: 14.44 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:54:05.86 +20:50:48.9: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.40 +/- 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
Gaia DR3 1262138335351551872,2461237.7413,13.46,0.05,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 1262138335351551872 20260716.2413 13.46CV 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 07 16.2413 2461237.7413 13.20 14:46:12.32 +20:58:06.5
25.93495 63.14917 galactic Boo Second-epoch detections are separated by 0.7" and 5.0 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 | 14:46:12.32 +20:58:06.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.358+/-0.037 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:46:12.32 +20:58:06.5: 14.09 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:46:12.32 +20:58:06.5: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461237.7413,13.20,0.05,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 20260716.2413 13.20CV 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 07 16.2413 2461237.7413 13.38 15:03:06.10 +17:56:22.3
23.05159 58.34711 galactic Boo Second-epoch detections are separated by 1.7" and 5.4 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 | 15:03:06.10 +17:56:22.3 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.033 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 15:03:06.10 +17:56:22.3: 14.23 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 15:03:06.10 +17:56:22.3: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461237.7413,13.38,0.05,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 20260716.2413 13.38CV 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 07 16.2413 2461237.7413 13.33 14:59:33.43 +17:41:46.4
21.98272 59.02708 galactic Boo Second-epoch detections are separated by 3.3" and 5.5 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 | 14:59:33.43 +17:41:46.4 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.033 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:59:33.43 +17:41:46.4: 14.24 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:59:33.43 +17:41:46.4: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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,2461237.7413,13.33,0.05,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 20260716.2413 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.16 14:49:23.74 +21:20:00.3
27.21058 62.55942 galactic Boo Second-epoch detections are separated by 2.0" 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 | 14:49:23.74 +21:20:00.3 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.034 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:49:23.74 +21:20:00.3: 14.23 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:49:23.74 +21:20:00.3: 14.15 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461237.7413,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.60 14:55:40.06 +18:35:49.5
22.91161 60.22909 galactic Boo Second-epoch detections are separated by 0.3" and 5.1 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 | 14:55:40.06 +18:35:49.5 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.041 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:55:40.06 +18:35:49.5: 14.77 +/- 0.10 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:55:40.06 +18:35:49.5: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.69 +/- 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,2461237.7413,13.60,0.05,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 20260716.2413 13.60CV 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 07 16.2413 2461237.7413 13.07 14:54:58.87 +18:25:04.1
22.45189 60.31064 galactic Boo Second-epoch detections are separated by 1.0" and 5.1 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 | 14:54:58.87 +18:25:04.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.459+/-0.028 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:54:58.87 +18:25:04.1: 14.09 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:54:58.87 +18:25:04.1: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461237.7413,13.07,0.05,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 20260716.2413 13.07CV 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 07 16.2413 2461237.7413 13.27 14:43:01.82 +21:54:59.9
27.44854 64.14597 galactic Boo Second-epoch detections are separated by 1.4" and 5.1 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 J220.7576+21.9164 | 14:43:01.82 +21:54:59.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.379+/-0.031 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:43:01.82 +21:54:59.9: 14.20 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:43:01.82 +21:54:59.9: 14.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 J220.7576+21.9164,2461237.7413,13.27,0.05,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
ATO J220.7576+21.9164 20260716.2413 13.27CV 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 07 16.2413 2461237.7413 13.28 14:54:03.28 +20:10:00.0
25.62234 61.14993 galactic Boo Second-epoch detections are separated by 2.5" and 5.2 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 | 14:54:03.28 +20:10:00.0 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:54:03.28 +20:10:00.0: 14.38 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:54:03.28 +20:10:00.0: 14.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461237.7413,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.28CV 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 07 16.2413 2461237.7413 13.28 14:43:34.40 +22:25:30.2
28.64861 64.17214 galactic Boo Second-epoch detections are separated by 1.2" and 4.9 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 | 14:43:34.40 +22:25:30.2 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.032 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:43:34.40 +22:25:30.2: 14.23 +/- 0.05 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:43:34.40 +22:25:30.2: 14.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461237.7413,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.28CV 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 07 16.2413 2461237.7413 13.29 14:53:29.30 +18:48:30.7
22.91141 60.78679 galactic Boo Second-epoch detections are separated by 1.2" and 4.9 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 | 14:53:29.30 +18:48:30.7 (user input) | T | P | (position from user input) J-Ks=0.670+/-0.032 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:53:29.30 +18:48:30.7: 14.20 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:53:29.30 +18:48:30.7: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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,2461237.7413,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.52 14:51:32.41 +20:07:46.9
25.12800 61.69190 galactic Boo Second-epoch detections are separated by 2.2" and 5.4 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 | 14:51:32.41 +20:07:46.9 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.039 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:51:32.41 +20:07:46.9: 14.52 +/- 0.08 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:51:32.41 +20:07:46.9: 14.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.48 +/- 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,2461237.7413,13.52,0.05,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 20260716.2413 13.52CV 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 07 16.2413 2461237.7413 13.41 14:50:46.58 +19:26:44.0
23.64630 61.61795 galactic Boo Second-epoch detections are separated by 1.1" and 5.2 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 | 14:50:46.58 +19:26:44.0 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.032 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:50:46.58 +19:26:44.0: 14.40 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:50:46.58 +19:26:44.0: 14.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461237.7413,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.42 14:51:25.73 +21:35:06.6
28.03923 62.18591 galactic Boo Second-epoch detections are separated by 1.4" and 5.0 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 | 14:51:25.73 +21:35:06.6 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.037 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:51:25.73 +21:35:06.6: 14.52 +/- 0.07 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:51:25.73 +21:35:06.6: 14.50 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.51 +/- 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,2461237.7413,13.42,0.05,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 20260716.2413 13.42CV 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 07 16.2413 2461237.7413 13.32 14:54:46.85 +18:02:45.5
21.72455 60.20895 galactic Boo Second-epoch detections are separated by 1.0" and 5.1 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 | 14:54:46.85 +18:02:45.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.624+/-0.029 (K)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:54:46.85 +18:02:45.5: 14.21 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:54:46.85 +18:02:45.5: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461237.7413,13.32,0.05,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 20260716.2413 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.18 14:42:11.28 +21:41:09.2
26.80763 64.26298 galactic Boo Second-epoch detections are separated by 0.9" and 4.9 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 | 14:42:11.28 +21:41:09.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.345+/-0.035 (G)
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:42:11.28 +21:41:09.2: 14.06 +/- 0.04 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:42:11.28 +21:41:09.2: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461237.7413,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.2413 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.2413 2461237.7413 13.27 14:41:57.97 +21:10:38.5
25.66061 64.15255 galactic Boo Second-epoch detections are separated by 0.5" and 5.0 pix
The object was found in VSX 1" Gaia DR3 1241377494235381120
Type: ROT
# Max. Min./Amp. JD0 Period
13.800 G 13.830 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits at 14:41:57.97 +21:10:38.5: 14.22 +/- 0.06 detection
Forced photometry on wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits at 14:41:57.97 +21:10:38.5: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 1241377494235381120,2461237.7413,13.27,0.05,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
Gaia DR3 1241377494235381120 20260716.2413 13.27CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461172.81834368 12.05.2026 07:38:14.894 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
First image: 2461172.81834368 12.05.2026 07:38:14.894 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
Last image: 2461237.74153520 16.07.2026 05:47:38.641 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 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): 6178
Objects passed selection criteria: 6158
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 4694.25
Average stars matched: 4597.75 (97.9443 %)
Memory usage VmPeak: 115484 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:30:20 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: 2461172.81834368 12.05.2026 07:38:14.894 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
First image: 2461172.81834368 12.05.2026 07:38:14.894 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
Last image: 2461237.74153520 16.07.2026 05:47:38.641 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 153
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.13
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 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): 35220
Objects passed selection criteria: 35119
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 27432.8
Average stars matched: 26551.5 (96.7876 %)
Memory usage VmPeak: 141608 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:32:01 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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
SExtractor catalog cache: saved Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.cat to cache
SExtractor catalog cache: saved Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.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: 2461237.74099413
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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits exists and is non-empty
Saving wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits to local_wcs_cache/
'wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits' -> 'local_wcs_cache/wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits'
wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits exists and is non-empty
Saving wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits to local_wcs_cache/
'wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits' -> 'local_wcs_cache/wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits'
wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits exists and is non-empty
Saving wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits to local_wcs_cache/
'wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits' -> 'local_wcs_cache/wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits'
wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits exists and is non-empty
Saving wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits to local_wcs_cache/
'wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits' -> 'local_wcs_cache/wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits (1st reference image)
verification OK: wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
Image size: 941.3'x626.7' 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: 14:46:00.692 +22:00:19.78 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits (1st new image)
verification OK: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
Image size: 941.2'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: 14:46:19.903 +21:59:54.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:46:00.692 +22:00:19.78
Second-epoch image center 14:46:19.903 +21:59:54.20
Angular distance between the image centers 0.0746 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits (2nd new image)
verification OK: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
Image size: 941.2'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: 14:46:21.202 +21:59:29.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:46:00.692 +22:00:19.78
Second-epoch image center 14:46:21.202 +21:59:29.77
Angular distance between the image centers 0.0804 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 14:46:19.903 +21:59:54.20
Second-epoch second image center 14:46:21.202 +21:59:29.77
Angular distance between the image centers 0.00844 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits &> /tmp/tmp.AVVpB93vrA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits &> /tmp/tmp.n8WMcGNnCq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits &> /tmp/tmp.VxA2ufoPZn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits &> /tmp/tmp.XgQvBiUl6Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits and wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits and wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat
Found non-empty wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits and wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat
The reference image (wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits) and catalog (wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat) found
'wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat' -> 'wcsmag.cat'
Read 6537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.9734 to 230.5645 deg, Dec +16.1049 to +27.5058 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 212.9734 to 230.5645 deg, Dec 16.1049 to 27.5058 deg
Loaded 4754 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): 3513 out of 3661 total matches.
Matched with Tycho-2 3661 out of 6537 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.833200
a=0.000000 b=1.000000 c=22.833200
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.9734 to 230.5645 deg, Dec +16.1049 to +27.5058 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 212.9734 to 230.5645 deg, Dec 16.1049 to 27.5058 deg
Loaded 4754 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): 3513 out of 3661 total matches.
Matched with Tycho-2 3661 out of 6537 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits:
Forced-photometry filter: calibrated wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits -> calib.txt_param_ref_wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits (aperture=6.2)
Read 6562 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.9733 to 230.5647 deg, Dec +16.1804 to +27.5059 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 212.9733 to 230.5647 deg, Dec 16.1804 to 27.5059 deg
Loaded 4728 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): 3504 out of 3660 total matches.
Matched with Tycho-2 3660 out of 6562 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits:
Forced-photometry filter: calibrated wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits -> calib.txt_param_ref_wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
2.1 pix Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
2.7 pix fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
2.7 pix fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
2.1 pix wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
2.1 pix wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
Limiting magnitude estimates:
15.4 mag. Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
15.4 mag. Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
14.0 mag. fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
14.0 mag. fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AVVpB93vrA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits' -> 'wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
WCS_IMAGE_NAME=wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
WCS-calibrated image found: wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
Checking if the catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits alredy exist and is non-empty...
Catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits
WCS catalog name: wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=408, bad_region=0, passed=6537
Got 6537 stars (including 6117 good ones) from the SExtractor catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat
util/solve_plate_with_UCAC5 got 6537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6487 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits N_match=962 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.499 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.313 n_q1=248 n_q2=219 n_q3=251 n_q4=244 worst_quadrant_to_overall_ratio=1.382
The image catalog is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits -region wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.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.n8WMcGNnCq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.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-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits' -> 'wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
WCS_IMAGE_NAME=wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
WCS-calibrated image found: wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
Checking if the catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits alredy exist and is non-empty...
Catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits
WCS catalog name: wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=415, bad_region=0, passed=6562
Got 6562 stars (including 6139 good ones) from the SExtractor catalog wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 6562 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
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(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6514 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
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(), 6514 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6514 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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=Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits N_match=963 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.469 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.350 n_q1=249 n_q2=220 n_q3=251 n_q4=243 worst_quadrant_to_overall_ratio=1.281
The image catalog is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits -region wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.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.VxA2ufoPZn (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_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.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_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
WCS_IMAGE_NAME=wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
WCS-calibrated image found: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
Checking if the catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat corresponding to the image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat corresponding to the image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
WCS catalog name: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=122, bad_region=0, passed=3101
Got 3101 stars (including 2976 good ones) from the SExtractor catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat
util/solve_plate_with_UCAC5 got 3101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits N_match=958 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.309 n_q1=335 n_q2=182 n_q3=343 n_q4=98 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits -region wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.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.XgQvBiUl6Y (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_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.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_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
WCS_IMAGE_NAME=wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
WCS-calibrated image found: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
Checking if the catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat corresponding to the image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat corresponding to the image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
WCS catalog name: wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=107, bad_region=0, passed=2686
Got 2686 stars (including 2575 good ones) from the SExtractor catalog wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat
util/solve_plate_with_UCAC5 got 2686 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 2521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 2519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 2519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits N_match=959 sigma_overall_arcsec=0.299 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.294 n_q1=322 n_q2=135 n_q3=379 n_q4=123 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits -region wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.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-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits sigma_overall=0.361 worst_q_ratio=1.382
ref2=Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits sigma_overall=0.366 worst_q_ratio=1.281
new1=fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits sigma_overall=0.306 worst_q_ratio=1.200
new2=fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits sigma_overall=0.299 worst_q_ratio=1.144
reference average sigma_overall=0.3635 worst_q_ratio=1.3315
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265_astrometric_residuals.png (962 matched stars from wcs_Boo-08-Q1b1x1_2026-05-12_02-38-14_20.00sec_-5.00C_LIGHTs_0265.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266_astrometric_residuals.png (963 matched stars from wcs_Boo-08-Q1b1x1_2026-05-12_02-38-56_20.00sec_-4.90C_LIGHTs_0266.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170_astrometric_residuals.png (958 matched stars from wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171_astrometric_residuals.png (959 matched stars from wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-46-51_20.00sec_0.00C_LIGHTs_0170.fits'
Saving fully-calibrated image wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-08-Q1b1x1_004907_TTUQ1b1x1_2290846_kBjpfKwH/wcs_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171.fits'
Preparing the HTML report for the field Boo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 05833_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 05833_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 52933_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52933_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 52934_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52934_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 52937_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52937_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 52938_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52938_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 52957_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52957_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 15:12:10.78 +18:57:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52961_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52961_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 52962_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52962_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 52967_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52967_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 52968_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52968_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 52972_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52972_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 52974_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52974_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 52975_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52975_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 52980_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52980_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 52989_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52989_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 52991_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52991_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 52993_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52993_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 52994_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52994_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 52996_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52996_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 52998_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52998_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 52999_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 52999_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 53001_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53001_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 53005_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53005_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 53007_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53007_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53009_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53009_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 53012_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53012_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 53014_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53014_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 53029_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53029_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 53051_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53051_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 14:38:07.84 +18:16:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53058_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53058_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 53069_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53069_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 53086_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53086_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 53087_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53087_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 53089_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53089_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 53091_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53091_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 53099_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53099_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 53101_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53101_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 53125_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53125_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53126_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53126_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 53128_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53128_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 53130_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53130_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 53133_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53133_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 53137_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53137_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 53156_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53156_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53159_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53159_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 53167_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53167_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 53184_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53184_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 53186_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53186_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53187_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53187_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 53188_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 53188_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 21805_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21805_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 19042_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 19042_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 33299_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 33299_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 23111_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 23111_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 18951_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 18951_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 37102_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 37102_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 19631_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 19631_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 35636_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 35636_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 37220_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 37220_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 19902_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 19902_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 27100_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 27100_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 31588_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 31588_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 28093_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 28093_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 21430_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21430_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 10656_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 10656_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 34738_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34738_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 32576_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 32576_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 35565_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 35565_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 22313_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22313_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 27313_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 27313_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 21867_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21867_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 18459_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 18459_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 18025_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 18025_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 13650_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 13650_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 10156_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 10156_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 14:52:05.97 +24:25:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37349_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 37349_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 22031_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22031_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 17410_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 17410_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 19828_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 19828_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 32392_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 32392_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 13808_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 13808_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 33481_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 33481_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 20075_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 20075_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
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Considering the candidate 22692_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22692_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 09197_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 09197_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 15:02:09.27 +24:29:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37595_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 37595_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 21582_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21582_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 19189_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 19189_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 21678_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21678_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 22870_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22870_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 27641_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 27641_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 35174_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 35174_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
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Considering the candidate 21396_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21396_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21422_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21422_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37675_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 37675_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35246_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 35246_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30491_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 30491_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30676_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 30676_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28033_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 28033_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17209_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 17209_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34200_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 34200_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 14:57:09.68 +19:15:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21660_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21660_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34256_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34256_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16150_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 16150_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30426_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 30426_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33691_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 33691_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34420_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34420_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34912_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34912_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34893_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34893_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06700_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 06700_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22023_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22023_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31225_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 31225_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31888_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 31888_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21155_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21155_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23375_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 23375_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27291_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 27291_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29800_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 29800_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28675_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 28675_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21898_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 21898_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31688_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 31688_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30965_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 30965_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20058_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 20058_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37249_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 37249_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18157_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 18157_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32329_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 32329_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36946_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 36946_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34417_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 34417_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20805_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 20805_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28182_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
The candidate 28182_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171 did not pass the final checks
**** FOUND 14:54:19.96 +17:41:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29610_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 29610_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20929_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 20929_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22888_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
Preparing report for the candidate 22888_fd_Boo-08-Q1b1x1_2026-07-16_00-47-38_20.00sec_0.00C_LIGHTs_0171
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 446s
Prepared the HTML report for the field Boo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:07:31.46 +25:03:07.4
15:09:14.81 +23:55:35.6
14:42:25.67 +22:42:03.4
14:41:35.97 +22:39:11.3
14:49:13.13 +22:22:29.6
14:43:34.40 +22:25:30.2
14:42:31.77 +22:13:00.0
14:50:47.14 +22:04:01.8
14:42:27.08 +22:09:23.1
14:48:41.41 +21:56:23.9
14:44:00.95 +21:57:50.3
14:49:02.91 +21:51:46.6
14:43:01.82 +21:54:59.9
14:51:25.73 +21:35:06.6
14:42:11.28 +21:41:09.2
14:45:19.01 +21:35:50.1
14:51:13.22 +21:25:54.9
14:50:19.32 +21:26:40.0
14:50:56.45 +21:25:35.0
14:49:50.37 +21:24:43.8
14:48:49.66 +21:24:23.3
14:47:39.32 +21:24:53.4
14:47:14.57 +21:23:23.3
14:49:54.86 +21:19:37.0
14:49:23.74 +21:20:00.3
14:47:24.46 +21:19:40.3
14:45:29.22 +21:21:01.6
14:49:19.28 +21:12:48.4
14:49:19.25 +21:07:14.4
14:50:05.56 +21:03:33.4
14:41:57.97 +21:10:38.5
14:52:32.93 +20:57:07.9
14:54:05.86 +20:50:48.9
14:46:04.65 +20:54:15.4
14:46:12.32 +20:58:06.5
14:52:10.85 +20:51:22.9
14:49:48.08 +20:37:48.1
14:46:44.84 +20:40:40.0
15:01:42.52 +17:30:57.6
14:59:33.43 +17:41:46.4
14:54:46.85 +18:02:45.5
15:03:06.10 +17:56:22.3
14:54:04.15 +18:17:36.3
14:56:24.00 +18:14:50.5
14:58:27.85 +18:16:20.5
14:54:58.87 +18:25:04.1
14:56:11.12 +18:27:34.6
14:56:05.44 +18:33:59.2
14:55:40.06 +18:35:49.5
15:00:05.12 +18:35:27.5
14:53:29.30 +18:48:30.7
14:59:47.41 +18:43:41.3
14:53:03.91 +18:51:25.7
14:55:48.70 +19:05:34.4
14:56:04.45 +19:08:14.6
14:50:53.85 +19:22:50.6
14:50:46.58 +19:26:44.0
14:50:35.15 +19:25:52.2
14:44:44.70 +19:38:15.1
14:48:37.68 +19:39:49.9
14:53:43.40 +19:30:08.2
14:55:39.73 +19:34:16.4
14:50:00.88 +19:39:05.3
14:46:35.12 +19:48:28.9
14:47:16.18 +19:52:46.5
14:51:32.41 +20:07:46.9
14:51:02.72 +20:09:49.6
14:52:19.68 +20:11:48.3
14:54:03.28 +20:10:00.0
14:47:51.84 +20:17:40.5
14:52:23.49 +20:17:33.7
########### Completed Boo-08-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 ####
14:47:14.57 +21:23:23.3
14:50:47.14 +22:04:01.8
14:52:32.93 +20:57:07.9
14:42:31.77 +22:13:00.0
14:51:02.72 +20:09:49.6
14:48:41.41 +21:56:23.9
14:47:16.18 +19:52:46.5
14:52:19.68 +20:11:48.3
14:49:02.91 +21:51:46.6
14:46:04.65 +20:54:15.4
14:56:05.44 +18:33:59.2
15:01:42.52 +17:30:57.6
14:50:56.45 +21:25:35.0
15:09:14.81 +23:55:35.6
14:44:44.70 +19:38:15.1
14:53:03.91 +18:51:25.7
14:46:35.12 +19:48:28.9
14:49:19.28 +21:12:48.4
14:52:10.85 +20:51:22.9
14:49:54.86 +21:19:37.0
14:49:13.13 +22:22:29.6
14:47:51.84 +20:17:40.5
14:45:29.22 +21:21:01.6
14:41:35.97 +22:39:11.3
14:44:00.95 +21:57:50.3
14:59:47.41 +18:43:41.3
14:55:48.70 +19:05:34.4
14:49:19.25 +21:07:14.4
14:52:23.49 +20:17:33.7
14:49:50.37 +21:24:43.8
14:42:27.08 +22:09:23.1
14:47:39.32 +21:24:53.4
14:50:05.56 +21:03:33.4
14:49:48.08 +20:37:48.1
14:55:39.73 +19:34:16.4
14:51:13.22 +21:25:54.9
14:50:19.32 +21:26:40.0
14:50:00.88 +19:39:05.3
14:56:24.00 +18:14:50.5
14:58:27.85 +18:16:20.5
14:46:44.84 +20:40:40.0
14:42:25.67 +22:42:03.4
14:48:49.66 +21:24:23.3
14:50:53.85 +19:22:50.6
14:54:04.15 +18:17:36.3
14:56:04.45 +19:08:14.6
14:50:35.15 +19:25:52.2
14:53:43.40 +19:30:08.2
14:48:37.68 +19:39:49.9
15:07:31.46 +25:03:07.4
14:47:24.46 +21:19:40.3
14:56:11.12 +18:27:34.6
15:00:05.12 +18:35:27.5
14:45:19.01 +21:35:50.1
14:54:05.86 +20:50:48.9
14:46:12.32 +20:58:06.5
15:03:06.10 +17:56:22.3
14:59:33.43 +17:41:46.4
14:49:23.74 +21:20:00.3
14:55:40.06 +18:35:49.5
14:54:58.87 +18:25:04.1
14:43:01.82 +21:54:59.9
14:54:03.28 +20:10:00.0
14:43:34.40 +22:25:30.2
14:53:29.30 +18:48:30.7
14:51:32.41 +20:07:46.9
14:50:46.58 +19:26:44.0
14:51:25.73 +21:35:06.6
14:54:46.85 +18:02:45.5
14:42:11.28 +21:41:09.2
14:41:57.97 +21:10:38.5
###################################################################################
14:47:14.57 +21:23:23.3 -- not an asteroid (will add it to exclusion list)
14:50:47.14 +22:04:01.8 -- not an asteroid (will add it to exclusion list)
14:52:32.93 +20:57:07.9 -- not an asteroid (will add it to exclusion list)
14:42:31.77 +22:13:00.0 -- not an asteroid (will add it to exclusion list)
14:51:02.72 +20:09:49.6 -- not an asteroid (will add it to exclusion list)
14:48:41.41 +21:56:23.9 -- not an asteroid (will add it to exclusion list)
14:47:16.18 +19:52:46.5 -- not an asteroid (will add it to exclusion list)
14:52:19.68 +20:11:48.3 -- not an asteroid (will add it to exclusion list)
14:49:02.91 +21:51:46.6 -- not an asteroid (will add it to exclusion list)
14:46:04.65 +20:54:15.4 -- not an asteroid (will add it to exclusion list)
14:56:05.44 +18:33:59.2 -- not an asteroid (will add it to exclusion list)
15:01:42.52 +17:30:57.6 -- not an asteroid (will add it to exclusion list)
14:50:56.45 +21:25:35.0 -- not an asteroid (will add it to exclusion list)
15:09:14.81 +23:55:35.6 -- not an asteroid (will add it to exclusion list)
14:44:44.70 +19:38:15.1 -- not an asteroid (will add it to exclusion list)
14:53:03.91 +18:51:25.7 -- not an asteroid (will add it to exclusion list)
14:46:35.12 +19:48:28.9 -- not an asteroid (will add it to exclusion list)
14:49:19.28 +21:12:48.4 -- not an asteroid (will add it to exclusion list)
14:52:10.85 +20:51:22.9 -- not an asteroid (will add it to exclusion list)
14:49:54.86 +21:19:37.0 -- not an asteroid (will add it to exclusion list)
14:49:13.13 +22:22:29.6 -- not an asteroid (will add it to exclusion list)
14:47:51.84 +20:17:40.5 -- not an asteroid (will add it to exclusion list)
14:45:29.22 +21:21:01.6 -- not an asteroid (will add it to exclusion list)
14:41:35.97 +22:39:11.3 -- not an asteroid (will add it to exclusion list)
14:44:00.95 +21:57:50.3 -- not an asteroid (will add it to exclusion list)
14:59:47.41 +18:43:41.3 -- not an asteroid (will add it to exclusion list)
14:55:48.70 +19:05:34.4 -- not an asteroid (will add it to exclusion list)
14:49:19.25 +21:07:14.4 -- not an asteroid (will add it to exclusion list)
14:52:23.49 +20:17:33.7 -- not an asteroid (will add it to exclusion list)
14:49:50.37 +21:24:43.8 -- not an asteroid (will add it to exclusion list)
14:42:27.08 +22:09:23.1 -- not an asteroid (will add it to exclusion list)
14:47:39.32 +21:24:53.4 -- not an asteroid (will add it to exclusion list)
14:50:05.56 +21:03:33.4 -- not an asteroid (will add it to exclusion list)
14:49:48.08 +20:37:48.1 -- not an asteroid (will add it to exclusion list)
14:55:39.73 +19:34:16.4 -- not an asteroid (will add it to exclusion list)
14:51:13.22 +21:25:54.9 -- not an asteroid (will add it to exclusion list)
14:50:19.32 +21:26:40.0 -- not an asteroid (will add it to exclusion list)
14:50:00.88 +19:39:05.3 -- not an asteroid (will add it to exclusion list)
14:56:24.00 +18:14:50.5 -- not an asteroid (will add it to exclusion list)
14:58:27.85 +18:16:20.5 -- not an asteroid (will add it to exclusion list)
14:46:44.84 +20:40:40.0 -- not an asteroid (will add it to exclusion list)
14:42:25.67 +22:42:03.4 -- not an asteroid (will add it to exclusion list)
14:48:49.66 +21:24:23.3 -- not an asteroid (will add it to exclusion list)
14:50:53.85 +19:22:50.6 -- not an asteroid (will add it to exclusion list)
14:54:04.15 +18:17:36.3 -- not an asteroid (will add it to exclusion list)
14:56:04.45 +19:08:14.6 -- not an asteroid (will add it to exclusion list)
14:50:35.15 +19:25:52.2 -- not an asteroid (will add it to exclusion list)
14:53:43.40 +19:30:08.2 -- not an asteroid (will add it to exclusion list)
14:48:37.68 +19:39:49.9 -- not an asteroid (will add it to exclusion list)
15:07:31.46 +25:03:07.4 -- not an asteroid (will add it to exclusion list)
14:47:24.46 +21:19:40.3 -- not an asteroid (will add it to exclusion list)
14:56:11.12 +18:27:34.6 -- not an asteroid (will add it to exclusion list)
15:00:05.12 +18:35:27.5 -- not an asteroid (will add it to exclusion list)
14:45:19.01 +21:35:50.1 -- not an asteroid (will add it to exclusion list)
14:54:05.86 +20:50:48.9 -- not an asteroid (will add it to exclusion list)
14:46:12.32 +20:58:06.5 -- not an asteroid (will add it to exclusion list)
15:03:06.10 +17:56:22.3 -- not an asteroid (will add it to exclusion list)
14:59:33.43 +17:41:46.4 -- not an asteroid (will add it to exclusion list)
14:49:23.74 +21:20:00.3 -- not an asteroid (will add it to exclusion list)
14:55:40.06 +18:35:49.5 -- not an asteroid (will add it to exclusion list)
14:54:58.87 +18:25:04.1 -- not an asteroid (will add it to exclusion list)
14:43:01.82 +21:54:59.9 -- not an asteroid (will add it to exclusion list)
14:54:03.28 +20:10:00.0 -- not an asteroid (will add it to exclusion list)
14:43:34.40 +22:25:30.2 -- not an asteroid (will add it to exclusion list)
14:53:29.30 +18:48:30.7 -- not an asteroid (will add it to exclusion list)
14:51:32.41 +20:07:46.9 -- not an asteroid (will add it to exclusion list)
14:50:46.58 +19:26:44.0 -- not an asteroid (will add it to exclusion list)
14:51:25.73 +21:35:06.6 -- not an asteroid (will add it to exclusion list)
14:54:46.85 +18:02:45.5 -- not an asteroid (will add it to exclusion list)
14:42:11.28 +21:41:09.2 -- not an asteroid (will add it to exclusion list)
14:41:57.97 +21:10:38.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
14:41:35.97 +22:39:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:41:57.97 +21:10:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:11.28 +21:41:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:25.67 +22:42:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:27.08 +22:09:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:42:31.77 +22:13:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:01.82 +21:54:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:43:34.40 +22:25:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:00.95 +21:57:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:44:44.70 +19:38:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:19.01 +21:35:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:45:29.22 +21:21:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:04.65 +20:54:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:12.32 +20:58:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:35.12 +19:48:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:46:44.84 +20:40:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:14.57 +21:23:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:16.18 +19:52:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:24.46 +21:19:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:39.32 +21:24:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:47:51.84 +20:17:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:48:37.68 +19:39:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:48:41.41 +21:56:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:48:49.66 +21:24:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:02.91 +21:51:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:13.13 +22:22:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:19.25 +21:07:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:19.28 +21:12:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:23.74 +21:20:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:48.08 +20:37:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:50.37 +21:24:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:49:54.86 +21:19:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:00.88 +19:39:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:05.56 +21:03:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:19.32 +21:26:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:35.15 +19:25:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:46.58 +19:26:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:47.14 +22:04:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:53.85 +19:22:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:50:56.45 +21:25:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:51:02.72 +20:09:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:51:13.22 +21:25:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:51:25.73 +21:35:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:51:32.41 +20:07:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:52:10.85 +20:51:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:52:19.68 +20:11:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:52:23.49 +20:17:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:52:32.93 +20:57:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:53:03.91 +18:51:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:53:29.30 +18:48:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:53:43.40 +19:30:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:03.28 +20:10:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:04.15 +18:17:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:05.86 +20:50:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:46.85 +18:02:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:58.87 +18:25:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:55:39.73 +19:34:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:55:40.06 +18:35:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:55:48.70 +19:05:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:56:04.45 +19:08:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:56:05.44 +18:33:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:56:11.12 +18:27:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:56:24.00 +18:14:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:58:27.85 +18:16:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:59:33.43 +17:41:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:59:47.41 +18:43:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:00:05.12 +18:35:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:01:42.52 +17:30:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:03:06.10 +17:56:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:07:31.46 +25:03:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:09:14.81 +23:55:35.6 -- 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)
14:41:35.97 +22:39:11.3 -- not a known variable star
14:41:57.97 +21:10:38.5 -- a known variable star
14:42:11.28 +21:41:09.2 -- not a known variable star
14:42:25.67 +22:42:03.4 -- a known variable star
14:42:27.08 +22:09:23.1 -- a known variable star
14:42:31.77 +22:13:00.0 -- not a known variable star
14:43:01.82 +21:54:59.9 -- not a known variable star
14:43:34.40 +22:25:30.2 -- not a known variable star
14:44:00.95 +21:57:50.3 -- not a known variable star
14:44:44.70 +19:38:15.1 -- not a known variable star
14:45:19.01 +21:35:50.1 -- not a known variable star
14:45:29.22 +21:21:01.6 -- not a known variable star
14:46:04.65 +20:54:15.4 -- not a known variable star
14:46:12.32 +20:58:06.5 -- not a known variable star
14:46:35.12 +19:48:28.9 -- a known variable star
14:46:44.84 +20:40:40.0 -- not a known variable star
14:47:14.57 +21:23:23.3 -- not a known variable star
14:47:16.18 +19:52:46.5 -- not a known variable star
14:47:24.46 +21:19:40.3 -- not a known variable star
14:47:39.32 +21:24:53.4 -- not a known variable star
14:47:51.84 +20:17:40.5 -- not a known variable star
14:48:37.68 +19:39:49.9 -- not a known variable star
14:48:41.41 +21:56:23.9 -- not a known variable star
14:48:49.66 +21:24:23.3 -- a known variable star
14:49:02.91 +21:51:46.6 -- not a known variable star
14:49:13.13 +22:22:29.6 -- not a known variable star
14:49:19.25 +21:07:14.4 -- not a known variable star
14:49:19.28 +21:12:48.4 -- not a known variable star
14:49:23.74 +21:20:00.3 -- not a known variable star
14:49:48.08 +20:37:48.1 -- not a known variable star
14:49:50.37 +21:24:43.8 -- not a known variable star
14:49:54.86 +21:19:37.0 -- a known variable star
14:50:00.88 +19:39:05.3 -- not a known variable star
14:50:05.56 +21:03:33.4 -- not a known variable star
14:50:19.32 +21:26:40.0 -- not a known variable star
14:50:35.15 +19:25:52.2 -- not a known variable star
14:50:46.58 +19:26:44.0 -- not a known variable star
14:50:47.14 +22:04:01.8 -- not a known variable star
14:50:53.85 +19:22:50.6 -- not a known variable star
14:50:56.45 +21:25:35.0 -- not a known variable star
14:51:02.72 +20:09:49.6 -- not a known variable star
14:51:13.22 +21:25:54.9 -- not a known variable star
14:51:25.73 +21:35:06.6 -- not a known variable star
14:51:32.41 +20:07:46.9 -- not a known variable star
14:52:10.85 +20:51:22.9 -- not a known variable star
14:52:19.68 +20:11:48.3 -- not a known variable star
14:52:23.49 +20:17:33.7 -- a known variable star
14:52:32.93 +20:57:07.9 -- not a known variable star
14:53:03.91 +18:51:25.7 -- not a known variable star
14:53:29.30 +18:48:30.7 -- not a known variable star
14:53:43.40 +19:30:08.2 -- not a known variable star
14:54:03.28 +20:10:00.0 -- not a known variable star
14:54:04.15 +18:17:36.3 -- not a known variable star
14:54:05.86 +20:50:48.9 -- a known variable star
14:54:46.85 +18:02:45.5 -- not a known variable star
14:54:58.87 +18:25:04.1 -- not a known variable star
14:55:39.73 +19:34:16.4 -- not a known variable star
14:55:40.06 +18:35:49.5 -- not a known variable star
14:55:48.70 +19:05:34.4 -- not a known variable star
14:56:04.45 +19:08:14.6 -- not a known variable star
14:56:05.44 +18:33:59.2 -- not a known variable star
14:56:11.12 +18:27:34.6 -- not a known variable star
14:56:24.00 +18:14:50.5 -- not a known variable star
14:58:27.85 +18:16:20.5 -- not a known variable star
14:59:33.43 +17:41:46.4 -- not a known variable star
14:59:47.41 +18:43:41.3 -- not a known variable star
15:00:05.12 +18:35:27.5 -- not a known variable star
15:01:42.52 +17:30:57.6 -- not a known variable star
15:03:06.10 +17:56:22.3 -- not a known variable star
15:07:31.46 +25:03:07.4 -- a known variable star
15:09:14.81 +23:55:35.6 -- not a known variable star
Found 62 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
71 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 71 (excluding asteroids and hot pixels, 62 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)2461237.74099413 -observatory V36
07:16:50.08 +17:17:33.1 Mercury (4.8mag)
10:35:55.17 +10:02:03.4 Venus (-4.1mag)
04:41:38.01 +22:05:57.2 Mars (1.3mag)
08:22:02.25 +19:54:17.0 Jupiter (-1.8mag)
00:56:23.41 +03:22:05.5 Saturn (0.7mag)
04:08:19.48 +20:47:59.3 Uranus (5.8mag)
00:16:57.84 +00:19:57.4 Neptune (7.7mag)
20:30:21.94 -23:20:36.1 Pluto (14.4mag)
09:23:23.97 +15:29:39.4 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 361 Jul 16 04:30 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461237.74099413:
08:22:04.36 +19:54:08.2 Io (6.1mag)
08:21:54.41 +19:54:47.5 Europa (6.3mag)
08:22:06.72 +19:54:04.4 Ganymede (5.6mag)
08:21:39.74 +19:55:40.0 Callisto (6.8mag)
08:20:18.07 +19:41:02.2 Himalia (15.7mag)
08:22:01.36 +19:54:21.4 Thebe (16.6mag)
08:19:38.83 +19:44:12.1 Elara (17.7mag)
08:25:44.85 +19:45:18.7 Pasiphae (17.9mag)
08:26:39.66 +20:00:14.7 Carme (19.0mag)
00:56:35.23 +03:21:50.1 Titan (8.5mag)
00:56:24.97 +03:21:50.4 Rhea (9.8mag)
00:55:48.63 +03:20:12.6 Iapetus (11.2mag)
00:56:10.20 +03:22:18.0 Hyperion (14.5mag)
00:56:16.26 +03:18:27.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 04:30 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.74099413:
17:55:15.64 -31:38:04.7 JWST
17:37:37.25 +38:01:48.0 Chandra
21:01:13.39 +42:46:47.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 04:30 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.74099413 -observatory V36
02:44:32.52 +15:06:49.5 17.8mag P/1996 R2 (Lagerkvist)
18:13:33.82 -34:30:22.0 13.8mag P/2010 H2 (Vales)
06:31:33.37 -68:14:35.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:49.70 +32:32:55.4 17.6mag C/2017 K2 (PANSTARRS)
02:18:45.10 +18:26:18.5 15.7mag P/2021 N1 (ZTF)
22:55:51.63 +32:15:05.3 17.3mag C/2022 E2 (ATLAS)
06:19:04.26 +26:52:10.1 16.7mag C/2022 N2 (PANSTARRS)
10:00:40.88 +29:30:58.0 16.9mag C/2022 QE78 (ATLAS)
09:13:33.52 +05:06:10.7 17.9mag C/2022 R6 (PANSTARRS)
18:03:42.33 +21:02:54.6 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.69 -11:31:50.9 17.7mag P/2023 B1 (PANSTARRS)
21:41:55.16 +67:32:21.9 17.8mag C/2023 H5 (Lemmon)
16:19:44.92 -10:41:22.1 14.0mag C/2023 R1 (PANSTARRS)
08:10:58.99 +66:01:57.6 17.9mag C/2024 A1 (ATLAS)
07:40:27.23 +30:17:50.2 14.8mag C/2024 E1 (Wierzchos)
15:13:38.29 +15:27:53.1 17.6mag C/2024 G6 (ATLAS)
19:33:41.28 +40:28:47.3 13.7mag C/2024 J3 (ATLAS)
21:41:13.89 +46:51:29.3 17.8mag C/2024 R4 (PANSTARRS)
04:55:09.29 -13:32:43.1 15.7mag C/2024 T5 (ATLAS)
06:39:23.53 +28:05:11.0 18.0mag C/2025 J1 (Borisov)
07:18:21.06 -13:26:00.7 16.8mag C/2025 R3 (PANSTARRS)
10:03:02.14 +22:10:28.4 17.6mag C/2025 V2 (Rankin)
12:46:43.23 +03:40:24.8 17.1mag C/2025 Y1 (ATLAS)
16:36:01.65 +79:09:35.4 17.2mag C/2026 A2 (Bok)
02:52:14.51 +45:29:10.4 16.8mag C/2026 B2 (Sun-Gao)
11:29:22.28 +05:32:47.2 17.0mag A/2026 E1
21:28:08.22 -17:17:28.2 7.1mag 10P/Tempel
11:16:17.28 -02:08:54.9 16.2mag 29P/Schwassmann-Wachmann
04:08:36.01 +30:11:07.7 17.9mag 47P/Ashbrook-Jackson
10:20:21.67 +12:07:37.4 17.1mag 63P/Wild
00:50:42.83 -05:02:52.3 15.5mag 65P/Gunn
04:41:36.99 +20:27:08.3 13.7mag 78P/Gehrels
02:31:37.80 +11:23:37.6 16.3mag 88P/Howell
06:52:54.92 +30:08:38.6 15.8mag 93P/Lovas
04:40:13.23 +31:18:22.5 16.7mag 114P/Wiseman-Skiff
08:23:05.00 +30:01:11.2 15.2mag 123P/West-Hartley
10:59:10.13 -01:12:07.3 16.9mag 124P/Mrkos
05:01:09.55 +20:58:00.5 16.2mag 128P/Shoemaker-Holt
05:47:18.83 +19:38:53.8 17.8mag 131P/Mueller
00:02:57.38 +03:08:43.2 17.9mag 139P/Vaisala-Oterma
07:34:45.34 +15:43:14.3 16.3mag 141P-D/Machholz
03:19:08.25 -20:38:07.5 15.2mag 161P/Hartley-IRAS
05:54:18.61 +35:08:12.9 15.4mag 162P/SidingSpring
18:47:00.01 +18:59:01.0 14.2mag 169P/NEAT
01:54:55.24 +08:13:12.5 17.6mag 220P/McNaught
16:35:30.25 -08:38:29.7 17.2mag 235P/LINEAR
08:57:38.15 +32:44:32.2 18.0mag 240P/NEAT
20:39:13.32 -50:46:53.1 17.8mag 259P/Garradd
02:15:52.09 +14:50:51.6 15.6mag 260P/McNaught
05:55:09.09 +37:16:07.4 17.4mag 295P/LINEAR
15:06:29.37 +05:31:07.8 17.6mag 391P/Kowalski
08:39:54.69 +19:25:59.5 17.9mag 450P/LONEOS
08:00:58.89 +38:43:26.0 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 04:30 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
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
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
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
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
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
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
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
-rw-r--r-- 1 apache apache 5.6K Jul 16 04:30 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +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
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 16 04:30 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:36:34.158 -10:42:13.45 AT 2026sta 2026-06-26.37 22.35
22:31:00.882 -14:40:17.84 AT 2026ssz 2026-06-26.40 22.03
21:55:03.781 -12:10:33.26 AT 2026ssy 2026-06-26.41 22.31
21:07:26.444 -20:35:07.74 AT 2026ssx 2026-06-27.33 21.66
21:00:47.829 -20:43:36.13 AT 2026ssw 2026-06-27.33 21.32
18:58:49.786 -21:29:54.27 AT 2026ssv 2026-07-06.26 21.93
21:15:32.626 -21:37:53.76 AT 2026ssu 2026-06-27.33 21.39
22:49:45.273 -15:16:33.71 AT 2026sst 2026-06-27.41 21.88
22:21:22.865 -18:28:38.60 AT 2026sss 2026-06-26.37 22.73
21:48:11.294 -15:58:33.77 AT 2026ssr 2026-06-26.41 21.95
21:56:29.244 -10:33:36.38 AT 2026ssq 2026-06-26.39 22.31
22:04:36.634 -18:37:38.63 AT 2026ssp 2026-06-26.37 22.56
21:52:03.725 -20:04:23.97 AT 2026sso 2026-06-26.39 22.15
22:28:31.768 -14:13:03.02 AT 2026ssn 2026-06-26.40 23.19
22:10:38.868 -20:00:07.81 AT 2026ssm 2026-06-26.37 21.5
00:37:08.843 -05:37:20.31 AT 2026ssl 2026-06-23.58 20.49
16:50:39.367 +12:02:04.48 AT 2026ssk 2026-06-23.30 21.04
21:28:51.588 -30:52:46.37 AT 2026ssj 2026-06-23.54 20.48
13:14:31.067 +38:32:01.92 AT 2026ssi 2026-06-11.32 19.048
00:23:13.025 -04:43:14.99 AT 2026ssh 2026-06-23.58 20.7
-rw-r--r-- 1 apache apache 89K Jul 16 04:30 tns_transients_list.txt
