This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m
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 16.3217 2461237.8217 11.65 16:22:57.54 +25:16:02.9
43.23132 42.87024 galactic Her Second-epoch detections are separated by 2.0" and 2.7 pix
The object was found in VSX 2" Gaia DR3 1302604589503290880
Type: ROT
# Max. Min./Amp. JD0 Period
12.540 G 12.570 G G
The object was not found in astcheck.
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:57.54 +25:16:02.9: 12.69 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:57.54 +25:16:02.9: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 57.54 +25 16 02.9 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1302604589503290880,2461237.8217,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1302604589503290880 20260716.3217 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.79 16:21:42.91 +25:22:08.5
43.27033 43.16774 galactic Her Second-epoch detections are separated by 0.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:21:42.91 +25:22:08.5 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.034 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:42.91 +25:22:08.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:42.91 +25:22:08.5: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 42.91 +25 22 08.5 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.88 16:29:34.49 +24:19:05.8
42.52245 41.17372 galactic Her Second-epoch detections are separated by 1.1" and 2.4 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 | 16:29:34.49 +24:19:05.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.414+/-0.034 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:29:34.49 +24:19:05.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:29:34.49 +24:19:05.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 29 34.49 +24 19 05.8 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 12.03 16:22:09.89 +23:53:48.4
41.36401 42.68840 galactic Her Second-epoch detections are separated by 1.1" and 2.3 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 | 16:22:09.89 +23:53:48.4 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:09.89 +23:53:48.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:09.89 +23:53:48.4: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 09.89 +23 53 48.4 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.77 17:04:38.33 +22:59:46.9
43.88099 33.10991 galactic Her Second-epoch detections are separated by 2.0" and 2.8 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 | 17:04:38.33 +22:59:46.9 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.030 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:04:38.33 +22:59:46.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:04:38.33 +22:59:46.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 04 38.33 +22 59 46.9 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.86 16:23:12.42 +23:46:38.1
41.29553 42.42661 galactic Her Second-epoch detections are separated by 1.8" and 2.2 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 | 16:23:12.42 +23:46:38.1 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.032 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:23:12.42 +23:46:38.1: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:23:12.42 +23:46:38.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 23 12.42 +23 46 38.1 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.45 17:06:35.21 +22:51:46.2
43.89897 32.64218 galactic Her Second-epoch detections are separated by 0.5" and 2.3 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 | 17:06:35.21 +22:51:46.2 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:35.21 +22:51:46.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:35.21 +22:51:46.2: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 06 35.21 +22 51 46.2 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.41 16:21:40.77 +20:29:10.3
36.91634 41.79091 galactic Her Second-epoch detections are separated by 1.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1202065894797853440 | 16:21:40.80 +20:29:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.352+/-0.030 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:40.77 +20:29:10.3: 12.57 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:40.77 +20:29:10.3: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 40.77 +20 29 10.3 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1202065894797853440,2461237.8217,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1202065894797853440 20260716.3217 11.41CV 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 16.3217 2461237.8217 11.56 16:22:32.20 +23:59:24.9
41.51753 42.63175 galactic Her Second-epoch detections are separated by 0.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:22:32.20 +23:59:24.9 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.331+/-0.033 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:32.20 +23:59:24.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:32.20 +23:59:24.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 32.20 +23 59 24.9 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.44 17:03:34.16 +23:04:34.2
43.87929 33.36857 galactic Her Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571287079303700480 | 17:03:34.14 +23:04:34.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.036 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:34.16 +23:04:34.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:34.16 +23:04:34.2: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 03 34.16 +23 04 34.2 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571287079303700480,2461237.8217,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571287079303700480 20260716.3217 11.44CV 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 16.3217 2461237.8217 11.22 16:26:40.61 +20:36:42.6
37.57111 40.72225 galactic Her Second-epoch detections are separated by 0.3" and 2.4 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 | ATO J246.6815+20.6130 | 16:26:40.61 +20:36:42.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.698+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:40.61 +20:36:42.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:40.61 +20:36:42.6: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 40.61 +20 36 42.6 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J246.6815+20.6130,2461237.8217,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J246.6815+20.6130 20260716.3217 11.22CV 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 16.3217 2461237.8217 11.58 16:26:24.67 +20:42:14.6
37.66041 40.81052 galactic Her Second-epoch detections are separated by 1.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1297399295299240064 | 16:26:24.65 +20:42:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.545+/-0.032 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:24.67 +20:42:14.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:24.67 +20:42:14.6: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 24.67 +20 42 14.6 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1297399295299240064,2461237.8217,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1297399295299240064 20260716.3217 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.55 16:22:23.98 +20:19:55.9
36.79332 41.58175 galactic Her Second-epoch detections are separated by 1.0" and 2.5 pix
The object was found in VSX 0" Gaia DR3 1202048306907902976
Type: VAR
# Max. Min./Amp. JD0 Period
12.260 G 12.280 G 0.065502700000 K
The object was not found in astcheck.
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:23.98 +20:19:55.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:23.98 +20:19:55.9: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 23.98 +20 19 55.9 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1202048306907902976,2461237.8217,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1202048306907902976 20260716.3217 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.93 16:26:25.29 +20:26:26.9
37.33206 40.72413 galactic Her Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:25.29 +20:26:26.9 (user input) | T | P | (position from user input) J-Ks=0.749+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:25.29 +20:26:26.9: 13.67 +/- 0.04 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:25.29 +20:26:26.9: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 25.29 +20 26 26.9 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.43 16:27:31.39 +20:40:55.0
37.74185 40.55693 galactic Her Second-epoch detections are separated by 0.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1297375410984331520 | 16:27:31.42 +20:40:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.319+/-0.028 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:31.39 +20:40:55.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:31.39 +20:40:55.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 27 31.39 +20 40 55.0 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1297375410984331520,2461237.8217,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1297375410984331520 20260716.3217 11.43CV 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 16.3217 2461237.8217 11.78 16:26:20.54 +20:21:24.4
37.21922 40.71465 galactic Her Second-epoch detections are separated by 1.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:20.54 +20:21:24.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.714+/-0.032 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:20.54 +20:21:24.4: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:20.54 +20:21:24.4: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 20.54 +20 21 24.4 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 10.94 17:04:01.15 +22:59:56.0
43.83030 33.24608 galactic Her Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571273713365591168 | 17:04:01.21 +22:59:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.877+/-0.029 (M)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:04:01.15 +22:59:56.0: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:04:01.15 +22:59:56.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 04 01.15 +22 59 56.0 10.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571273713365591168,2461237.8217,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571273713365591168 20260716.3217 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.63 16:26:06.14 +20:26:59.8
37.31179 40.79787 galactic Her Second-epoch detections are separated by 1.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:06.14 +20:26:59.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.267+/-0.034 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:06.14 +20:26:59.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:06.14 +20:26:59.8: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 06.14 +20 26 59.8 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 10.98 16:26:36.80 +24:14:41.2
42.18574 41.80400 galactic Her Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1302263362941387648 | 16:26:36.78 +24:14:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.278+/-0.025 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:36.80 +24:14:41.2: 11.89 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:36.80 +24:14:41.2: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 36.80 +24 14 41.2 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1302263362941387648,2461237.8217,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1302263362941387648 20260716.3217 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 10.84 16:22:03.36 +24:01:46.8
41.52914 42.74807 galactic Her Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1302198972791859968 | 16:22:03.35 +24:01:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.031 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:03.36 +24:01:46.8: 11.86 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:03.36 +24:01:46.8: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 03.36 +24 01 46.8 10.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1302198972791859968,2461237.8217,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1302198972791859968 20260716.3217 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.84 16:26:28.42 +24:22:19.8
42.33909 41.86870 galactic Her Second-epoch detections are separated by 1.0" and 2.5 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 | 16:26:28.42 +24:22:19.8 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:28.42 +24:22:19.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:28.42 +24:22:19.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 28.42 +24 22 19.8 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.97 16:23:10.85 +23:49:19.3
41.35171 42.44455 galactic Her Second-epoch detections are separated by 1.3" and 2.4 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 | 16:23:10.85 +23:49:19.3 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:23:10.85 +23:49:19.3: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:23:10.85 +23:49:19.3: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 23 10.85 +23 49 19.3 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.44 16:45:00.86 +23:17:39.5
42.54276 37.49702 galactic Her Second-epoch detections are separated by 2.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1299484587821405568 | 16:45:00.89 +23:17:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:45:00.86 +23:17:39.5: 12.39 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:45:00.86 +23:17:39.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 45 00.86 +23 17 39.5 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1299484587821405568,2461237.8217,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1299484587821405568 20260716.3217 11.44CV 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 16.3217 2461237.8217 11.77 16:26:51.63 +20:21:58.5
37.28265 40.60274 galactic Her Second-epoch detections are separated by 1.0" and 2.5 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 | 16:26:51.63 +20:21:58.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.498+/-0.031 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:51.63 +20:21:58.5: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:51.63 +20:21:58.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 51.63 +20 21 58.5 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 10.95 17:03:51.93 +23:07:28.0
43.95968 33.31898 galactic Her Second-epoch detections are separated by 1.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571287452961999360 | 17:03:51.91 +23:07:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.032 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:51.93 +23:07:28.0: 11.82 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:51.93 +23:07:28.0: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 03 51.93 +23 07 28.0 10.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571287452961999360,2461237.8217,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571287452961999360 20260716.3217 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.86 16:34:45.74 +17:47:20.9
34.97125 37.97071 galactic Her Second-epoch detections are separated by 2.0" and 2.4 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 | 16:34:45.74 +17:47:20.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.303+/-0.033 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:34:45.74 +17:47:20.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:34:45.74 +17:47:20.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 34 45.74 +17 47 20.9 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.10 16:22:10.76 +23:56:14.7
41.41847 42.69617 galactic Her Second-epoch detections are separated by 1.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1302193234715540480 | 16:22:10.78 +23:56:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.420+/-0.029 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:10.76 +23:56:14.7: 12.38 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:10.76 +23:56:14.7: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 10.76 +23 56 14.7 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1302193234715540480,2461237.8217,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1302193234715540480 20260716.3217 11.10CV 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 16.3217 2461237.8217 11.84 16:26:35.61 +20:44:16.2
37.72060 40.78082 galactic Her Second-epoch detections are separated by 0.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:35.61 +20:44:16.2 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.035 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:35.61 +20:44:16.2: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:35.61 +20:44:16.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 35.61 +20 44 16.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.37 17:05:32.03 +23:06:16.2
44.08065 32.94846 galactic Her Second-epoch detections are separated by 1.1" and 2.3 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 | Gaia DR3 4571367034414399744 | 17:05:31.98 +23:06:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.028 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:32.03 +23:06:16.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:32.03 +23:06:16.2: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 05 32.03 +23 06 16.2 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571367034414399744,2461237.8217,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571367034414399744 20260716.3217 11.37CV 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 16.3217 2461237.8217 11.85 16:27:16.21 +20:21:42.5
37.31787 40.51042 galactic Her Second-epoch detections are separated by 0.6" and 2.5 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 | 16:27:16.21 +20:21:42.5 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.032 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:16.21 +20:21:42.5: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:16.21 +20:21:42.5: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 27 16.21 +20 21 42.5 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.39 17:06:28.02 +22:35:02.0
43.57465 32.57940 galactic Her Second-epoch detections are separated by 2.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4568197176750123520 | 17:06:27.91 +22:35:02.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.244+/-0.028 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:28.02 +22:35:02.0: 12.32 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:28.02 +22:35:02.0: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 06 28.02 +22 35 02.0 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4568197176750123520,2461237.8217,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4568197176750123520 20260716.3217 11.39CV 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 16.3217 2461237.8217 11.21 17:06:43.50 +22:55:32.0
43.98159 32.63190 galactic Her Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571301918412553600 | 17:06:43.51 +22:55:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.306+/-0.028 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:43.50 +22:55:32.0: 12.31 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:43.50 +22:55:32.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 06 43.50 +22 55 32.0 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571301918412553600,2461237.8217,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571301918412553600 20260716.3217 11.21CV 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 16.3217 2461237.8217 11.69 16:27:49.49 +20:39:51.5
37.74943 40.48443 galactic Her Second-epoch detections are separated by 1.0" and 2.4 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 | 16:27:49.49 +20:39:51.5 (user input) | T | P | (position from user input) J-Ks=0.318+/-0.028 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:49.49 +20:39:51.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:49.49 +20:39:51.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 27 49.49 +20 39 51.5 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.48 17:05:46.71 +22:51:11.1
43.81774 32.81567 galactic Her Second-epoch detections are separated by 1.1" and 2.1 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 | 17:05:46.71 +22:51:11.1 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.031 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:46.71 +22:51:11.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:46.71 +22:51:11.1: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 05 46.71 +22 51 11.1 11.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.48CV 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 16.3217 2461237.8217 11.76 16:22:11.17 +25:20:31.2
43.27054 43.05796 galactic Her Second-epoch detections are separated by 0.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:22:11.17 +25:20:31.2 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.536+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:11.17 +25:20:31.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:11.17 +25:20:31.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 22 11.17 +25 20 31.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.85 16:28:04.48 +20:36:47.2
37.71019 40.41269 galactic Her Second-epoch detections are separated by 0.4" and 2.5 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 | 16:28:04.48 +20:36:47.2 (user input) | T | P | (position from user input) J-Ks=0.623+/-0.026 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:28:04.48 +20:36:47.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:28:04.48 +20:36:47.2: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 28 04.48 +20 36 47.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.18 17:06:12.46 +22:55:04.9
43.92826 32.74250 galactic Her Second-epoch detections are separated by 0.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571314154776976128 | 17:06:12.42 +22:55:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.558+/-0.029 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:12.46 +22:55:04.9: 12.22 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:12.46 +22:55:04.9: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 06 12.46 +22 55 04.9 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571314154776976128,2461237.8217,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571314154776976128 20260716.3217 11.18CV 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 16.3217 2461237.8217 12.04 16:26:15.85 +20:28:09.8
37.35218 40.76821 galactic Her Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:15.85 +20:28:09.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:15.85 +20:28:09.8: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:15.85 +20:28:09.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 15.85 +20 28 09.8 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 10.57 17:03:47.81 +23:02:09.7
43.85328 33.30630 galactic Her Second-epoch detections are separated by 0.4" and 2.3 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 | Gaia DR3 4571285773633790464 | 17:03:47.84 +23:02:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.802+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:47.81 +23:02:09.7: 11.49 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:47.81 +23:02:09.7: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 03 47.81 +23 02 09.7 10.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571285773633790464,2461237.8217,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571285773633790464 20260716.3217 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.92 16:28:23.89 +20:39:40.4
37.80178 40.35633 galactic Her Second-epoch detections are separated by 0.5" and 2.3 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 | 16:28:23.89 +20:39:40.4 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.494+/-0.026 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:28:23.89 +20:39:40.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:28:23.89 +20:39:40.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 28 23.89 +20 39 40.4 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.58 17:05:33.94 +23:00:31.1
43.97499 32.91134 galactic Her Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4571318033129846400 | 17:05:33.93 +23:00:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.714+/-0.027 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:33.94 +23:00:31.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:33.94 +23:00:31.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 17 05 33.94 +23 00 31.1 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4571318033129846400,2461237.8217,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4571318033129846400 20260716.3217 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.74 16:21:44.58 +25:20:52.5
43.24442 43.15643 galactic Her Second-epoch detections are separated by 2.3" and 2.3 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 | Gaia DR3 1303370536790688384 | 16:21:44.51 +25:20:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.684+/-0.032 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:44.58 +25:20:52.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:44.58 +25:20:52.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 44.58 +25 20 52.5 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303370536790688384,2461237.8217,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303370536790688384 20260716.3217 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.76 16:21:24.29 +25:17:38.0
43.14666 43.21708 galactic Her Second-epoch detections are separated by 4.5" and 2.0 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 | 16:21:24.29 +25:17:38.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.318+/-0.032 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:24.29 +25:17:38.0: 12.71 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:24.29 +25:17:38.0: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 24.29 +25 17 38.0 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.41 16:21:12.46 +23:52:54.4
41.26396 42.89505 galactic Her Second-epoch detections are separated by 0.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:21:12.46 +23:52:54.4 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.030 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:12.46 +23:52:54.4: 12.69 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:12.46 +23:52:54.4: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 12.46 +23 52 54.4 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.41CV 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 16.3217 2461237.8217 11.64 16:26:17.41 +20:40:20.3
37.60875 40.82726 galactic Her Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1297398848622640768 | 16:26:17.36 +20:40:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.578+/-0.029 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:17.41 +20:40:20.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:17.41 +20:40:20.3: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 17.41 +20 40 20.3 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1297398848622640768,2461237.8217,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1297398848622640768 20260716.3217 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.84 16:43:52.85 +23:23:31.2
42.56395 37.77443 galactic Her Second-epoch detections are separated by 0.3" and 2.4 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 | 16:43:52.85 +23:23:31.2 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.029 (G)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:43:52.85 +23:23:31.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:43:52.85 +23:23:31.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 43 52.85 +23 23 31.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.98 16:21:22.30 +20:28:23.0
36.86878 41.85505 galactic Her Second-epoch detections are separated by 1.7" and 2.3 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 | 16:21:22.30 +20:28:23.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.507+/-0.030 (K)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:22.30 +20:28:23.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:22.30 +20:28:23.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 21 22.30 +20 28 23.0 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3217 2461237.8217 11.35 16:26:55.33 +20:36:52.9
37.59884 40.66876 galactic Her Second-epoch detections are separated by 0.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:26:55.33 +20:36:52.9 (user input) | T | P | (position from user input) J-Ks=0.212+/-0.042 (F)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:55.33 +20:36:52.9: 12.65 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:55.33 +20:36:52.9: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3217* 16 26 55.33 +20 36 52.9 11.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8217,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3217 11.35CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461209.78738564 18.06.2026 06:53:40.119 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
First image: 2461209.78738564 18.06.2026 06:53:40.119 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Last image: 2461237.82193156 16.07.2026 07:43:24.887 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 5 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): 8458
Objects passed selection criteria: 8392
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 4858.75
Average stars matched: 4729.75 (97.345 %)
Memory usage VmPeak: 118176 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 03:37:22 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: 2461209.78738564 18.06.2026 06:53:40.119 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
First image: 2461209.78738564 18.06.2026 06:53:40.119 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Last image: 2461237.82193156 16.07.2026 07:43:24.887 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 286
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.05
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: 16 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): 53183
Objects passed selection criteria: 52986
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 32663.8
Average stars matched: 31424 (96.2045 %)
Memory usage VmPeak: 160612 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 03:39:52 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.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/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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: 2461237.82147957
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_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits exists and is non-empty
Saving wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits to local_wcs_cache/
'wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits'
wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits'
wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits exists and is non-empty
Saving wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits to local_wcs_cache/
'wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits'
wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits exists and is non-empty
Saving wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits to local_wcs_cache/
'wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:36:55.253 +22:00:26.08 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits (1st new image)
verification OK: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:37:14.188 +22:01:23.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:36:55.253 +22:00:26.08
Second-epoch image center 16:37:14.188 +22:01:23.78
Angular distance between the image centers 0.0749 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits (2nd new image)
verification OK: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:37:13.498 +22:01:12.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:36:55.253 +22:00:26.08
Second-epoch image center 16:37:13.498 +22:01:12.86
Angular distance between the image centers 0.0717 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 16:37:14.188 +22:01:23.78
Second-epoch second image center 16:37:13.498 +22:01:12.86
Angular distance between the image centers 0.00404 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/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits &> /tmp/tmp.6YD3JxbjKI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits &> /tmp/tmp.j6mEsHzsOW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits &> /tmp/tmp.W2yMh3VJ6B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits &> /tmp/tmp.h5JN37ioRD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits) and catalog (wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat) found
'wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 11249 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.5440 to 257.9495 deg, Dec +16.6160 to +27.2612 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 240.5440 to 257.9495 deg, Dec 16.6160 to 27.2612 deg
Loaded 7256 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): 5769 out of 6010 total matches.
Matched with Tycho-2 6010 out of 11249 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774500
a=0.000000 b=1.000000 c=22.774500
From vast_summary.log: estimated ref. image limiting mag.: -7.37
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 11249 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.5440 to 257.9495 deg, Dec +16.6160 to +27.2612 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 240.5440 to 257.9495 deg, Dec 16.6160 to 27.2612 deg
Loaded 7256 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): 5769 out of 6010 total matches.
Matched with Tycho-2 6010 out of 11249 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits:
Forced-photometry filter: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits (aperture=6.2)
Read 11287 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.5439 to 257.9495 deg, Dec +16.6161 to +27.2613 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 240.5439 to 257.9495 deg, Dec 16.6161 to 27.2613 deg
Loaded 7256 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): 5768 out of 6015 total matches.
Matched with Tycho-2 6015 out of 11287 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
2.2 pix Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
2.3 pix fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
2.3 pix fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
2.2 pix wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
2.2 pix wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Limiting magnitude estimates:
15.4 mag. Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
15.4 mag. Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
11.3 mag. fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
11.6 mag. fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 11.3 (SNR ) 9.6 (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.6YD3JxbjKI (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits' -> 'wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Checking if the catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS catalog name: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=651, bad_region=2261, passed=11249
Got 11249 stars (including 8441 good ones) from the SExtractor catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 11249 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 9139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 9139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 9140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits N_match=983 sigma_overall_arcsec=0.430 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.461 sigma_q4_arcsec=0.481 n_q1=312 n_q2=173 n_q3=323 n_q4=175 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits -region wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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.j6mEsHzsOW (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits' -> 'wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Checking if the catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS catalog name: wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=657, bad_region=2280, passed=11287
Got 11287 stars (including 8448 good ones) from the SExtractor catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 11287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 9145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 9145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 9146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits N_match=982 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.395 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.428 n_q1=313 n_q2=171 n_q3=327 n_q4=171 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits -region wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.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.W2yMh3VJ6B (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=26, bad_region=184, passed=947
Got 947 stars (including 742 good ones) from the SExtractor catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 718 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 719 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 719 stars left (next iteration limit 789)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits N_match=719 sigma_overall_arcsec=0.620 sigma_q1_arcsec=0.610 sigma_q2_arcsec=0.542 sigma_q3_arcsec=0.676 sigma_q4_arcsec=0.611 n_q1=201 n_q2=131 n_q3=212 n_q4=175 worst_quadrant_to_overall_ratio=1.090
The image catalog is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits -region wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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.h5JN37ioRD (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=35, bad_region=234, passed=1020
Got 1020 stars (including 756 good ones) from the SExtractor catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 1020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 587 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 735 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 735 matched stars entering correct_measured_positions(), 716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 735 matched stars entering correct_measured_positions(), 784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 533 to 587 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 735 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 734 stars left (next iteration limit 808)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits N_match=734 sigma_overall_arcsec=0.569 sigma_q1_arcsec=0.574 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.628 sigma_q4_arcsec=0.587 n_q1=200 n_q2=117 n_q3=241 n_q4=176 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits -region wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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=Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits sigma_overall=0.430 worst_q_ratio=1.120
ref2=Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits sigma_overall=0.415 worst_q_ratio=1.044
new1=fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits sigma_overall=0.620 worst_q_ratio=1.090
new2=fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits sigma_overall=0.569 worst_q_ratio=1.102
reference average sigma_overall=0.4225 worst_q_ratio=1.082
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224_astrometric_residuals.png (983 matched stars from wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225_astrometric_residuals.png (982 matched stars from wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228_astrometric_residuals.png (719 matched stars from wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229_astrometric_residuals.png (734 matched stars from wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits'
Preparing the HTML report for the field Her-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Her-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Creating symlink local_wcs_cache/wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits exists and is non-empty
wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits exists and is non-empty
wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:36:55.253 +22:00:26.08 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits (1st new image)
verification OK: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:37:14.188 +22:01:23.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:36:55.253 +22:00:26.08
Second-epoch image center 16:37:14.188 +22:01:23.78
Angular distance between the image centers 0.0749 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits (2nd new image)
verification OK: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:37:13.498 +22:01:12.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:36:55.253 +22:00:26.08
Second-epoch image center 16:37:13.498 +22:01:12.86
Angular distance between the image centers 0.0717 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 16:37:14.188 +22:01:23.78
Second-epoch second image center 16:37:13.498 +22:01:12.86
Angular distance between the image centers 0.00404 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/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits &> /tmp/tmp.cXs5BiaRf1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits &> /tmp/tmp.FrJNVY61sL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits &> /tmp/tmp.fxABQDHjuY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits &> /tmp/tmp.jf81JOkOSH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits and wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits) and catalog (wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat) found
'wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 67516 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.4969 to 257.9962 deg, Dec +16.6160 to +27.2709 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 240.4969 to 257.9962 deg, Dec 16.6160 to 27.2709 deg
Loaded 7301 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): 5326 out of 6047 total matches.
Matched with Tycho-2 6047 out of 67516 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.643300
a=0.000000 b=1.000000 c=22.643300
From vast_summary.log: estimated ref. image limiting mag.: -7.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 67516 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.4969 to 257.9962 deg, Dec +16.6160 to +27.2709 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 240.4969 to 257.9962 deg, Dec 16.6160 to 27.2709 deg
Loaded 7301 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): 5326 out of 6047 total matches.
Matched with Tycho-2 6047 out of 67516 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits:
Forced-photometry filter: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits (aperture=4.7)
Read 67317 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.4605 to 257.9752 deg, Dec +16.6092 to +27.2701 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 240.4605 to 257.9752 deg, Dec 16.6092 to 27.2701 deg
Loaded 7304 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): 5331 out of 6054 total matches.
Matched with Tycho-2 6054 out of 67317 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 102 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
2.1 pix Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
2.1 pix fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
2.1 pix fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
2.1 pix wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
2.1 pix wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Limiting magnitude estimates:
15.6 mag. Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
15.6 mag. Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
12.2 mag. fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
12.4 mag. fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cXs5BiaRf1 (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits' -> 'wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
Checking if the catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits
WCS catalog name: wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3792, bad_region=9139, passed=67492
Got 67492 stars (including 55005 good ones) from the SExtractor catalog wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 67492 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 59225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 59226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 59225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits N_match=982 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.458 sigma_q4_arcsec=0.494 n_q1=314 n_q2=181 n_q3=305 n_q4=182 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits -region wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.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.FrJNVY61sL (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits' -> 'wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
Checking if the catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits
WCS catalog name: wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3759, bad_region=9183, passed=67293
Got 67293 stars (including 54810 good ones) from the SExtractor catalog wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 67293 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 58853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 58852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 58852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits N_match=983 sigma_overall_arcsec=0.428 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.447 n_q1=313 n_q2=184 n_q3=308 n_q4=178 worst_quadrant_to_overall_ratio=1.046
The image catalog is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits -region wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.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.fxABQDHjuY (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=171, bad_region=1095, passed=8548
Got 8548 stars (including 7349 good ones) from the SExtractor catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 8548 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7565 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 533 to 588 (Dec 16.7 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits N_match=966 sigma_overall_arcsec=0.566 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.536 sigma_q3_arcsec=0.602 sigma_q4_arcsec=0.508 n_q1=283 n_q2=158 n_q3=294 n_q4=231 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits -region wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.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.jf81JOkOSH (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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.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_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=192, bad_region=1320, passed=8889
Got 8889 stars (including 7454 good ones) from the SExtractor catalog wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 8889 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 533 to 588 (Dec 16.7 to 27.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits N_match=969 sigma_overall_arcsec=0.526 sigma_q1_arcsec=0.513 sigma_q2_arcsec=0.491 sigma_q3_arcsec=0.579 sigma_q4_arcsec=0.524 n_q1=266 n_q2=145 n_q3=331 n_q4=227 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits -region wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-42-45_20.00sec_4.90C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-06-Q2b1x1_024412_TTUQ2b1x1_2032627_SrTOBT7m/wcs_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229.fits
Preparing the HTML report for the field Her-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:42.91 +25:22:08.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:57.54 +25:16:02.9: 12.69 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:04:38.33 +22:59:46.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:29:34.49 +24:19:05.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:23:12.42 +23:46:38.1: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:09.89 +23:53:48.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:35.21 +22:51:46.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:40.77 +20:29:10.3: 12.57 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:42.91 +25:22:08.5: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 16:21:42.91 +25:22:08.5: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7497 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:29:34.49 +24:19:05.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:04:38.33 +22:59:46.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:57.54 +25:16:02.9: 12.67 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:23:12.42 +23:46:38.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 16:29:34.49 +24:19:05.8: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8636 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 17:04:38.33 +22:59:46.9: ref_mag=12.97 +/- 0.01 new_mean_mag=11.7649 delta=1.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 16:22:57.54 +25:16:02.9: ref_mag=12.68 +/- 0.01 new_mean_mag=11.5967 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 16:23:12.42 +23:46:38.1: ref_mag=13.01 +/- 0.01 new_mean_mag=11.8199 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:09.89 +23:53:48.4: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 16:22:09.89 +23:53:48.4: ref_mag=13.70 +/- 0.03 new_mean_mag=12.0267 delta=1.67 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:32.20 +23:59:24.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:35.21 +22:51:46.2: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:35.21 +22:51:46.2: ref_mag=12.94 +/- 0.01 new_mean_mag=11.4397 delta=1.50 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:40.77 +20:29:10.3: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 16:21:40.77 +20:29:10.3: ref_mag=12.57 +/- 0.01 new_mean_mag=11.3826 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:34.16 +23:04:34.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:32.20 +23:59:24.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 16:22:32.20 +23:59:24.9: ref_mag=12.97 +/- 0.01 new_mean_mag=11.5569 delta=1.41 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:34.16 +23:04:34.2: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 17:03:34.16 +23:04:34.2: ref_mag=12.51 +/- 0.01 new_mean_mag=11.4372 delta=1.07 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:40.61 +20:36:42.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:40.61 +20:36:42.6: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:40.61 +20:36:42.6: ref_mag=12.54 +/- 0.01 new_mean_mag=11.2109 delta=1.33 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:24.67 +20:42:14.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:24.67 +20:42:14.6: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:24.67 +20:42:14.6: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5605 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:23.98 +20:19:55.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:23.98 +20:19:55.9: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 16:22:23.98 +20:19:55.9: ref_mag=12.51 +/- 0.01 new_mean_mag=11.4854 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:25.29 +20:26:26.9: 13.67 +/- 0.04 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:31.39 +20:40:55.0: 12.48 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:20.54 +20:21:24.4: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:04:01.15 +22:59:56.0: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:25.29 +20:26:26.9: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 16:26:25.29 +20:26:26.9: ref_mag=13.64 +/- 0.02 new_mean_mag=11.9115 delta=1.73 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:06.14 +20:26:59.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:31.39 +20:40:55.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 16:27:31.39 +20:40:55.0: ref_mag=12.47 +/- 0.01 new_mean_mag=11.3731 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:20.54 +20:21:24.4: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 16:26:20.54 +20:21:24.4: ref_mag=13.30 +/- 0.02 new_mean_mag=11.7695 delta=1.53 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:04:01.15 +22:59:56.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 17:04:01.15 +22:59:56.0: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9187 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:06.14 +20:26:59.8: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 16:26:06.14 +20:26:59.8: ref_mag=13.22 +/- 0.02 new_mean_mag=11.5433 delta=1.67 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:36.80 +24:14:41.2: 11.89 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:03.36 +24:01:46.8: 11.86 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:36.80 +24:14:41.2: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.00
Forced photometry filter KEPT candidate at 16:26:36.80 +24:14:41.2: ref_mag=11.90 +/- 0.00 new_mean_mag=10.9442 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:28.42 +24:22:19.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:03.36 +24:01:46.8: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.00
Forced photometry filter KEPT candidate at 16:22:03.36 +24:01:46.8: ref_mag=11.85 +/- 0.00 new_mean_mag=10.8130 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:28.42 +24:22:19.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:28.42 +24:22:19.8: ref_mag=12.86 +/- 0.01 new_mean_mag=11.7967 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:23:10.85 +23:49:19.3: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:23:10.85 +23:49:19.3: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 16:23:10.85 +23:49:19.3: ref_mag=13.22 +/- 0.02 new_mean_mag=11.9301 delta=1.29 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:45:00.86 +23:17:39.5: 12.39 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:51.63 +20:21:58.5: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:45:00.86 +23:17:39.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 16:45:00.86 +23:17:39.5: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3870 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:51.63 +20:21:58.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 16:26:51.63 +20:21:58.5: ref_mag=13.21 +/- 0.02 new_mean_mag=11.7744 delta=1.44 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:51.93 +23:07:28.0: 11.82 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:34:45.74 +17:47:20.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:10.76 +23:56:14.7: 12.38 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:51.93 +23:07:28.0: 11.84 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:34:45.74 +17:47:20.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.00
Forced photometry filter KEPT candidate at 17:03:51.93 +23:07:28.0: ref_mag=11.83 +/- 0.00 new_mean_mag=10.9231 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 16:34:45.74 +17:47:20.9: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8407 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:10.76 +23:56:14.7: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 16:22:10.76 +23:56:14.7: ref_mag=12.39 +/- 0.01 new_mean_mag=11.0606 delta=1.32 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:35.61 +20:44:16.2: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:35.61 +20:44:16.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:35.61 +20:44:16.2: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8560 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:32.03 +23:06:16.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:16.21 +20:21:42.5: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:28.02 +22:35:02.0: 12.32 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:43.50 +22:55:32.0: 12.31 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:32.03 +23:06:16.2: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:32.03 +23:06:16.2: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3542 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:16.21 +20:21:42.5: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 16:27:16.21 +20:21:42.5: ref_mag=13.17 +/- 0.02 new_mean_mag=11.7966 delta=1.37 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:43.50 +22:55:32.0: 12.31 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:28.02 +22:35:02.0: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:43.50 +22:55:32.0: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2014 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:28.02 +22:35:02.0: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3877 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:27:49.49 +20:39:51.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:27:49.49 +20:39:51.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 16:27:49.49 +20:39:51.5: ref_mag=12.80 +/- 0.01 new_mean_mag=11.6919 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:46.71 +22:51:11.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:46.71 +22:51:11.1: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:46.71 +22:51:11.1: ref_mag=12.72 +/- 0.01 new_mean_mag=11.4827 delta=1.24 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:22:11.17 +25:20:31.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:28:04.48 +20:36:47.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:22:11.17 +25:20:31.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 16:22:11.17 +25:20:31.2: ref_mag=12.75 +/- 0.01 new_mean_mag=11.6941 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:28:04.48 +20:36:47.2: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 16:28:04.48 +20:36:47.2: ref_mag=13.12 +/- 0.02 new_mean_mag=11.7942 delta=1.33 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:06:12.46 +22:55:04.9: 12.22 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:15.85 +20:28:09.8: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:03:47.81 +23:02:09.7: 11.49 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:06:12.46 +22:55:04.9: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:12.46 +22:55:04.9: ref_mag=12.22 +/- 0.01 new_mean_mag=11.1671 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:15.85 +20:28:09.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter KEPT candidate at 16:26:15.85 +20:28:09.8: ref_mag=13.63 +/- 0.02 new_mean_mag=12.0040 delta=1.63 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:03:47.81 +23:02:09.7: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.00
Forced photometry filter KEPT candidate at 17:03:47.81 +23:02:09.7: ref_mag=11.49 +/- 0.00 new_mean_mag=10.5331 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:28:23.89 +20:39:40.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 17:05:33.94 +23:00:31.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:28:23.89 +20:39:40.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter KEPT candidate at 16:28:23.89 +20:39:40.4: ref_mag=13.09 +/- 0.01 new_mean_mag=11.9145 delta=1.17 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 17:05:33.94 +23:00:31.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:33.94 +23:00:31.1: ref_mag=12.74 +/- 0.01 new_mean_mag=11.5930 delta=1.15 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:44.58 +25:20:52.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:44.58 +25:20:52.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 16:21:44.58 +25:20:52.5: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7093 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:24.29 +25:17:38.0: 12.71 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:24.29 +25:17:38.0: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 16:21:24.29 +25:17:38.0: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7371 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:12.46 +23:52:54.4: 12.69 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:12.46 +23:52:54.4: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 16:21:12.46 +23:52:54.4: ref_mag=12.70 +/- 0.01 new_mean_mag=11.3712 delta=1.33 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:17.41 +20:40:20.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:43:52.85 +23:23:31.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:17.41 +20:40:20.3: 12.65 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:43:52.85 +23:23:31.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:17.41 +20:40:20.3: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6309 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 16:43:52.85 +23:23:31.2: ref_mag=13.05 +/- 0.01 new_mean_mag=11.8297 delta=1.22 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:21:22.30 +20:28:23.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:21:22.30 +20:28:23.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 16:21:22.30 +20:28:23.0: ref_mag=13.37 +/- 0.02 new_mean_mag=11.9333 delta=1.44 (need > 0.90)
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-53-40_20.00sec_4.90C_LIGHT_0224.fits at 16:26:55.33 +20:36:52.9: 12.65 +/- 0.01 detection
Forced photometry on wcs_Her-06-Q2b1x1_2026-06-18_01-54-22_20.00sec_4.90C_LIGHT_0225.fits at 16:26:55.33 +20:36:52.9: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 16:26:55.33 +20:36:52.9: ref_mag=12.65 +/- 0.01 new_mean_mag=11.3470 delta=1.30 (need > 0.90)
Adding exclusion_list_local.txt__out10694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67163.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 82s
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: 23s
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Considering the candidate 82262_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82262_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 82267_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82267_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 82268_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82268_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 82271_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82271_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 82279_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82279_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 82283_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82283_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 82286_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82286_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 82287_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82287_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 82295_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82295_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 82304_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82304_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 82305_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82305_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 82312_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82312_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 82314_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82314_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 82317_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82317_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 82318_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82318_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 82339_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82339_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 82349_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82349_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 82356_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82356_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 82357_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82357_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 82359_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82359_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 82369_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82369_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 82371_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82371_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 82373_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82373_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 82376_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82376_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 82378_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82378_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 82385_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82385_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 82386_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82386_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 82388_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82388_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 82390_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82390_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 82392_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82392_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 82398_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82398_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 82400_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82400_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 82402_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82402_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 82404_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82404_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 82405_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82405_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 82411_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82411_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 82412_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82412_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 82415_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82415_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 82417_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82417_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 82420_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82420_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 82422_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82422_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 82423_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82423_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 82424_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 82424_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 11431_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 11431_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 10694_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 10694_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 17551_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 17551_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 20138_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 20138_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25357_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25357_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 20930_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 20930_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 07867_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 07867_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 29355_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 29355_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 17:02:30.81 +22:25:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26109_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26109_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 67163_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 67163_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 19519_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 19519_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 24892_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 24892_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 47743_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47743_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 48303_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48303_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 47021_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47021_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 16258_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 16258_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 66903_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66903_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 19765_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 19765_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 48122_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48122_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 66166_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66166_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25295_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25295_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66805_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66805_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 17895_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 17895_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 19183_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 19183_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 17188_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 17188_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 20660_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 20660_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 24275_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 24275_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 66438_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66438_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 24412_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 24412_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 51112_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 51112_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 19790_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 19790_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48382_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48382_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 28745_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 28745_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 17:02:31.72 +22:31:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14645_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 14645_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 24510_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 24510_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 66271_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66271_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 27980_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 27980_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25652_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25652_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 48015_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48015_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 26226_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26226_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 10867_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 10867_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 47633_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47633_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25778_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25778_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 67100_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 67100_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25054_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25054_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 47921_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47921_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
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Considering the candidate 25212_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25212_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51509_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 51509_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 16:27:01.81 +17:50:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10845_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 10845_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11192_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 11192_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20118_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 20118_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48118_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48118_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23676_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 23676_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66532_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 66532_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51580_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 51580_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 16:26:06.77 +17:51:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47666_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47666_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34234_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 34234_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 16:30:13.23 +21:29:25.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66935_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 66935_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 16:30:33.47 +20:28:46.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59511_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229
The candidate 59511_fd_Her-06-Q2b1x1_2026-07-16_02-43-24_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 16:21:55.27 +19:09:15.7 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 110s
Prepared the HTML report for the field Her-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:21:42.91 +25:22:08.5
16:21:44.58 +25:20:52.5
16:22:11.17 +25:20:31.2
16:21:24.29 +25:17:38.0
16:22:57.54 +25:16:02.9
16:26:28.42 +24:22:19.8
16:29:34.49 +24:19:05.8
16:26:36.80 +24:14:41.2
16:22:03.36 +24:01:46.8
16:22:32.20 +23:59:24.9
16:22:10.76 +23:56:14.7
16:21:12.46 +23:52:54.4
16:22:09.89 +23:53:48.4
16:23:10.85 +23:49:19.3
16:23:12.42 +23:46:38.1
16:43:52.85 +23:23:31.2
16:45:00.86 +23:17:39.5
17:03:51.93 +23:07:28.0
17:05:32.03 +23:06:16.2
17:03:34.16 +23:04:34.2
17:03:47.81 +23:02:09.7
17:05:33.94 +23:00:31.1
17:04:01.15 +22:59:56.0
17:04:38.33 +22:59:46.9
17:06:43.50 +22:55:32.0
17:06:12.46 +22:55:04.9
17:06:35.21 +22:51:46.2
17:05:46.71 +22:51:11.1
17:06:28.02 +22:35:02.0
16:22:23.98 +20:19:55.9
16:28:04.48 +20:36:47.2
16:26:55.33 +20:36:52.9
16:26:40.61 +20:36:42.6
16:28:23.89 +20:39:40.4
16:27:49.49 +20:39:51.5
16:26:17.41 +20:40:20.3
16:27:31.39 +20:40:55.0
16:26:24.67 +20:42:14.6
16:26:35.61 +20:44:16.2
16:34:45.74 +17:47:20.9
16:26:20.54 +20:21:24.4
16:27:16.21 +20:21:42.5
16:26:51.63 +20:21:58.5
16:21:22.30 +20:28:23.0
16:26:06.14 +20:26:59.8
16:26:25.29 +20:26:26.9
16:26:15.85 +20:28:09.8
16:21:40.77 +20:29:10.3
########### Completed Her-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
16:22:57.54 +25:16:02.9
16:21:42.91 +25:22:08.5
16:29:34.49 +24:19:05.8
16:22:09.89 +23:53:48.4
17:04:38.33 +22:59:46.9
16:23:12.42 +23:46:38.1
17:06:35.21 +22:51:46.2
16:21:40.77 +20:29:10.3
16:22:32.20 +23:59:24.9
17:03:34.16 +23:04:34.2
16:26:40.61 +20:36:42.6
16:26:24.67 +20:42:14.6
16:22:23.98 +20:19:55.9
16:26:25.29 +20:26:26.9
16:27:31.39 +20:40:55.0
16:26:20.54 +20:21:24.4
17:04:01.15 +22:59:56.0
16:26:06.14 +20:26:59.8
16:26:36.80 +24:14:41.2
16:22:03.36 +24:01:46.8
16:26:28.42 +24:22:19.8
16:23:10.85 +23:49:19.3
16:45:00.86 +23:17:39.5
16:26:51.63 +20:21:58.5
17:03:51.93 +23:07:28.0
16:34:45.74 +17:47:20.9
16:22:10.76 +23:56:14.7
16:26:35.61 +20:44:16.2
17:05:32.03 +23:06:16.2
16:27:16.21 +20:21:42.5
17:06:28.02 +22:35:02.0
17:06:43.50 +22:55:32.0
16:27:49.49 +20:39:51.5
17:05:46.71 +22:51:11.1
16:22:11.17 +25:20:31.2
16:28:04.48 +20:36:47.2
17:06:12.46 +22:55:04.9
16:26:15.85 +20:28:09.8
17:03:47.81 +23:02:09.7
16:28:23.89 +20:39:40.4
17:05:33.94 +23:00:31.1
16:21:44.58 +25:20:52.5
16:21:24.29 +25:17:38.0
16:21:12.46 +23:52:54.4
16:26:17.41 +20:40:20.3
16:43:52.85 +23:23:31.2
16:21:22.30 +20:28:23.0
16:26:55.33 +20:36:52.9
###################################################################################
16:22:57.54 +25:16:02.9 -- not an asteroid (will add it to exclusion list)
16:21:42.91 +25:22:08.5 -- not an asteroid (will add it to exclusion list)
16:29:34.49 +24:19:05.8 -- not an asteroid (will add it to exclusion list)
16:22:09.89 +23:53:48.4 -- not an asteroid (will add it to exclusion list)
17:04:38.33 +22:59:46.9 -- not an asteroid (will add it to exclusion list)
16:23:12.42 +23:46:38.1 -- not an asteroid (will add it to exclusion list)
17:06:35.21 +22:51:46.2 -- not an asteroid (will add it to exclusion list)
16:21:40.77 +20:29:10.3 -- not an asteroid (will add it to exclusion list)
16:22:32.20 +23:59:24.9 -- not an asteroid (will add it to exclusion list)
17:03:34.16 +23:04:34.2 -- not an asteroid (will add it to exclusion list)
16:26:40.61 +20:36:42.6 -- not an asteroid (will add it to exclusion list)
16:26:24.67 +20:42:14.6 -- not an asteroid (will add it to exclusion list)
16:22:23.98 +20:19:55.9 -- not an asteroid (will add it to exclusion list)
16:26:25.29 +20:26:26.9 -- not an asteroid (will add it to exclusion list)
16:27:31.39 +20:40:55.0 -- not an asteroid (will add it to exclusion list)
16:26:20.54 +20:21:24.4 -- not an asteroid (will add it to exclusion list)
17:04:01.15 +22:59:56.0 -- not an asteroid (will add it to exclusion list)
16:26:06.14 +20:26:59.8 -- not an asteroid (will add it to exclusion list)
16:26:36.80 +24:14:41.2 -- not an asteroid (will add it to exclusion list)
16:22:03.36 +24:01:46.8 -- not an asteroid (will add it to exclusion list)
16:26:28.42 +24:22:19.8 -- not an asteroid (will add it to exclusion list)
16:23:10.85 +23:49:19.3 -- not an asteroid (will add it to exclusion list)
16:45:00.86 +23:17:39.5 -- not an asteroid (will add it to exclusion list)
16:26:51.63 +20:21:58.5 -- not an asteroid (will add it to exclusion list)
17:03:51.93 +23:07:28.0 -- not an asteroid (will add it to exclusion list)
16:34:45.74 +17:47:20.9 -- not an asteroid (will add it to exclusion list)
16:22:10.76 +23:56:14.7 -- not an asteroid (will add it to exclusion list)
16:26:35.61 +20:44:16.2 -- not an asteroid (will add it to exclusion list)
17:05:32.03 +23:06:16.2 -- not an asteroid (will add it to exclusion list)
16:27:16.21 +20:21:42.5 -- not an asteroid (will add it to exclusion list)
17:06:28.02 +22:35:02.0 -- not an asteroid (will add it to exclusion list)
17:06:43.50 +22:55:32.0 -- not an asteroid (will add it to exclusion list)
16:27:49.49 +20:39:51.5 -- not an asteroid (will add it to exclusion list)
17:05:46.71 +22:51:11.1 -- not an asteroid (will add it to exclusion list)
16:22:11.17 +25:20:31.2 -- not an asteroid (will add it to exclusion list)
16:28:04.48 +20:36:47.2 -- not an asteroid (will add it to exclusion list)
17:06:12.46 +22:55:04.9 -- not an asteroid (will add it to exclusion list)
16:26:15.85 +20:28:09.8 -- not an asteroid (will add it to exclusion list)
17:03:47.81 +23:02:09.7 -- not an asteroid (will add it to exclusion list)
16:28:23.89 +20:39:40.4 -- not an asteroid (will add it to exclusion list)
17:05:33.94 +23:00:31.1 -- not an asteroid (will add it to exclusion list)
16:21:44.58 +25:20:52.5 -- not an asteroid (will add it to exclusion list)
16:21:24.29 +25:17:38.0 -- not an asteroid (will add it to exclusion list)
16:21:12.46 +23:52:54.4 -- not an asteroid (will add it to exclusion list)
16:26:17.41 +20:40:20.3 -- not an asteroid (will add it to exclusion list)
16:43:52.85 +23:23:31.2 -- not an asteroid (will add it to exclusion list)
16:21:22.30 +20:28:23.0 -- not an asteroid (will add it to exclusion list)
16:26:55.33 +20:36:52.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:21:12.46 +23:52:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:22.30 +20:28:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:24.29 +25:17:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:40.77 +20:29:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:42.91 +25:22:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:44.58 +25:20:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:03.36 +24:01:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:09.89 +23:53:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:10.76 +23:56:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:11.17 +25:20:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:23.98 +20:19:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:32.20 +23:59:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:57.54 +25:16:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:10.85 +23:49:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:12.42 +23:46:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:06.14 +20:26:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:15.85 +20:28:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:17.41 +20:40:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:20.54 +20:21:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:24.67 +20:42:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:25.29 +20:26:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:28.42 +24:22:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:35.61 +20:44:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:36.80 +24:14:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:40.61 +20:36:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:51.63 +20:21:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:55.33 +20:36:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:16.21 +20:21:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:31.39 +20:40:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:49.49 +20:39:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:28:04.48 +20:36:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:28:23.89 +20:39:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:34.49 +24:19:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:45.74 +17:47:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:52.85 +23:23:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:00.86 +23:17:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:34.16 +23:04:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:47.81 +23:02:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:51.93 +23:07:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:01.15 +22:59:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:38.33 +22:59:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:32.03 +23:06:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:33.94 +23:00:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:46.71 +22:51:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:12.46 +22:55:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:28.02 +22:35:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:35.21 +22:51:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:43.50 +22:55:32.0 -- 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)
16:21:12.46 +23:52:54.4 -- not a known variable star
16:21:22.30 +20:28:23.0 -- not a known variable star
16:21:24.29 +25:17:38.0 -- not a known variable star
16:21:40.77 +20:29:10.3 -- not a known variable star
16:21:42.91 +25:22:08.5 -- not a known variable star
16:21:44.58 +25:20:52.5 -- not a known variable star
16:22:03.36 +24:01:46.8 -- not a known variable star
16:22:09.89 +23:53:48.4 -- not a known variable star
16:22:10.76 +23:56:14.7 -- not a known variable star
16:22:11.17 +25:20:31.2 -- not a known variable star
16:22:23.98 +20:19:55.9 -- a known variable star
16:22:32.20 +23:59:24.9 -- not a known variable star
16:22:57.54 +25:16:02.9 -- a known variable star
16:23:10.85 +23:49:19.3 -- not a known variable star
16:23:12.42 +23:46:38.1 -- not a known variable star
16:26:06.14 +20:26:59.8 -- not a known variable star
16:26:15.85 +20:28:09.8 -- not a known variable star
16:26:17.41 +20:40:20.3 -- not a known variable star
16:26:20.54 +20:21:24.4 -- not a known variable star
16:26:24.67 +20:42:14.6 -- not a known variable star
16:26:25.29 +20:26:26.9 -- not a known variable star
16:26:28.42 +24:22:19.8 -- not a known variable star
16:26:35.61 +20:44:16.2 -- not a known variable star
16:26:36.80 +24:14:41.2 -- not a known variable star
16:26:40.61 +20:36:42.6 -- not a known variable star
16:26:51.63 +20:21:58.5 -- not a known variable star
16:26:55.33 +20:36:52.9 -- not a known variable star
16:27:16.21 +20:21:42.5 -- not a known variable star
16:27:31.39 +20:40:55.0 -- not a known variable star
16:27:49.49 +20:39:51.5 -- not a known variable star
16:28:04.48 +20:36:47.2 -- not a known variable star
16:28:23.89 +20:39:40.4 -- not a known variable star
16:29:34.49 +24:19:05.8 -- not a known variable star
16:34:45.74 +17:47:20.9 -- not a known variable star
16:43:52.85 +23:23:31.2 -- not a known variable star
16:45:00.86 +23:17:39.5 -- not a known variable star
17:03:34.16 +23:04:34.2 -- not a known variable star
17:03:47.81 +23:02:09.7 -- not a known variable star
17:03:51.93 +23:07:28.0 -- not a known variable star
17:04:01.15 +22:59:56.0 -- not a known variable star
17:04:38.33 +22:59:46.9 -- not a known variable star
17:05:32.03 +23:06:16.2 -- not a known variable star
17:05:33.94 +23:00:31.1 -- not a known variable star
17:05:46.71 +22:51:11.1 -- not a known variable star
17:06:12.46 +22:55:04.9 -- not a known variable star
17:06:28.02 +22:35:02.0 -- not a known variable star
17:06:35.21 +22:51:46.2 -- not a known variable star
17:06:43.50 +22:55:32.0 -- not a known variable star
Found 46 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
48 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 48 (excluding asteroids and hot pixels, 46 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)2461237.82147957 -observatory V36
07:16:39.34 +17:17:59.7 Mercury (4.8mag)
10:36:14.89 +09:59:49.4 Venus (-4.1mag)
04:41:52.43 +22:06:28.1 Mars (1.3mag)
08:22:06.70 +19:54:02.5 Jupiter (-1.8mag)
00:56:23.77 +03:22:06.3 Saturn (0.7mag)
04:08:20.36 +20:48:01.6 Uranus (5.8mag)
00:16:57.77 +00:19:56.6 Neptune (7.7mag)
20:30:21.48 -23:20:38.2 Pluto (14.4mag)
09:29:17.19 +14:59:00.5 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 361 Jul 16 03:37 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461237.82147957:
08:22:07.00 +19:54:00.7 Io (6.0mag)
08:21:58.36 +19:54:35.1 Europa (6.3mag)
08:22:12.27 +19:53:45.6 Ganymede (5.6mag)
08:21:43.75 +19:55:27.4 Callisto (6.8mag)
08:20:22.31 +19:40:50.0 Himalia (15.7mag)
08:22:04.76 +19:54:11.0 Thebe (16.6mag)
08:19:43.07 +19:43:58.9 Elara (17.7mag)
08:25:49.42 +19:45:01.7 Pasiphae (17.9mag)
08:26:43.82 +20:00:01.0 Carme (19.0mag)
00:56:35.66 +03:21:51.7 Titan (8.5mag)
00:56:25.86 +03:21:51.3 Rhea (9.8mag)
00:55:48.98 +03:20:12.7 Iapetus (11.2mag)
00:56:10.44 +03:22:18.0 Hyperion (14.5mag)
00:56:16.50 +03:18:27.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 03:37 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.82147957:
17:55:00.30 -31:35:44.9 JWST
17:40:26.70 +36:04:07.0 Chandra
02:26:26.72 +62:53:46.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 03:37 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.82147957 -observatory V36
02:44:39.22 +15:07:22.5 17.8mag P/1996 R2 (Lagerkvist)
18:13:30.30 -34:30:27.5 13.8mag P/2010 H2 (Vales)
06:31:38.22 -68:14:41.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:51.35 +32:33:00.5 17.6mag C/2017 K2 (PANSTARRS)
02:19:08.45 +18:33:28.2 15.7mag P/2021 N1 (ZTF)
22:55:48.45 +32:15:02.3 17.3mag C/2022 E2 (ATLAS)
06:19:09.72 +26:52:07.0 16.7mag C/2022 N2 (PANSTARRS)
10:00:45.19 +29:30:44.7 16.9mag C/2022 QE78 (ATLAS)
09:13:36.71 +05:06:15.2 17.9mag C/2022 R6 (PANSTARRS)
18:03:39.50 +21:02:41.2 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.43 -11:31:58.4 17.8mag P/2023 B1 (PANSTARRS)
21:41:48.82 +67:32:15.4 17.8mag C/2023 H5 (Lemmon)
16:19:36.22 -10:41:51.7 14.0mag C/2023 R1 (PANSTARRS)
08:11:07.70 +66:02:14.0 17.9mag C/2024 A1 (ATLAS)
07:40:33.47 +30:18:04.1 14.8mag C/2024 E1 (Wierzchos)
15:13:36.23 +15:27:58.4 17.6mag C/2024 G6 (ATLAS)
19:33:34.80 +40:29:36.6 13.7mag C/2024 J3 (ATLAS)
21:41:08.34 +46:52:09.5 17.8mag C/2024 R4 (PANSTARRS)
04:55:13.80 -13:32:31.9 15.7mag C/2024 T5 (ATLAS)
06:39:27.47 +28:04:22.5 18.0mag C/2025 J1 (Borisov)
07:18:24.32 -13:26:29.0 16.8mag C/2025 R3 (PANSTARRS)
10:03:08.01 +22:10:14.6 17.6mag C/2025 V2 (Rankin)
12:46:45.11 +03:40:10.9 17.1mag C/2025 Y1 (ATLAS)
16:35:49.11 +79:09:31.7 17.2mag C/2026 A2 (Bok)
02:52:19.11 +45:29:22.7 16.8mag C/2026 B2 (Sun-Gao)
11:29:25.61 +05:33:33.6 17.0mag A/2026 E1
21:28:14.97 -17:19:25.3 7.1mag 10P/Tempel
11:16:19.71 -02:09:08.4 16.2mag 29P/Schwassmann-Wachmann
04:08:42.89 +30:11:38.6 17.9mag 47P/Ashbrook-Jackson
10:20:31.79 +12:06:03.9 17.1mag 63P/Wild
00:50:44.51 -05:02:51.8 15.5mag 65P/Gunn
04:41:48.68 +20:27:19.9 13.7mag 78P/Gehrels
02:31:45.18 +11:24:14.5 16.3mag 88P/Howell
06:53:09.09 +30:08:16.6 15.8mag 93P/Lovas
04:40:29.19 +31:18:27.9 16.7mag 114P/Wiseman-Skiff
08:23:16.87 +30:00:35.5 15.2mag 123P/West-Hartley
10:59:19.31 -01:14:04.2 16.9mag 124P/Mrkos
05:01:17.29 +20:58:07.3 16.2mag 128P/Shoemaker-Holt
05:47:27.90 +19:38:49.4 17.8mag 131P/Mueller
00:02:58.30 +03:08:52.2 17.9mag 139P/Vaisala-Oterma
07:35:02.25 +15:42:08.7 16.3mag 141P-D/Machholz
03:19:09.95 -20:37:46.3 15.2mag 161P/Hartley-IRAS
05:54:36.18 +35:09:06.3 15.4mag 162P/SidingSpring
18:46:42.08 +19:02:31.7 14.2mag 169P/NEAT
01:55:06.43 +08:13:40.6 17.6mag 220P/McNaught
16:35:30.11 -08:38:43.6 17.2mag 235P/LINEAR
08:57:48.27 +32:44:03.7 18.0mag 240P/NEAT
20:39:10.00 -50:47:48.1 17.8mag 259P/Garradd
02:16:05.80 +14:53:07.4 15.6mag 260P/McNaught
05:55:23.95 +37:16:25.5 17.4mag 295P/LINEAR
15:06:29.44 +05:30:40.3 17.6mag 391P/Kowalski
08:39:59.10 +19:25:47.2 17.9mag 450P/LONEOS
08:01:06.47 +38:43:01.4 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 03:37 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
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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 03:37 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
21:26:53.186 +04:17:24.51 AT 2026ssg 2026-06-23.48 20.92
22:34:24.397 -29:59:37.51 AT 2026ssf 2026-06-25.56 20.68
22:26:15.310 -27:42:10.55 AT 2026sse 2026-06-25.56 21.41
22:13:00.422 -28:48:04.48 AT 2026ssd 2026-06-25.55 21.47
22:13:31.243 -26:34:31.26 AT 2026ssc 2026-06-25.55 21.32
-rw-r--r-- 1 apache apache 89K Jul 16 03:37 tns_transients_list.txt
