This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws
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 16.3749 2461237.8749 12.47 17:04:28.50 +33:25:21.0
56.09974 35.83062 galactic Her Second-epoch detections are separated by 0.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:04:28.50 +33:25:21.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.371+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:28.50 +33:25:21.0: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:28.50 +33:25:21.0: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 16.3749* 17 04 28.50 +33 25 21.0 12.5 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,2461237.8749,12.47,0.05,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 20260716.3749 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.62 17:12:01.08 +32:54:16.1
55.88051 34.17897 galactic Her Second-epoch detections are separated by 2.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:12:01.08 +32:54:16.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.452+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:01.08 +32:54:16.1: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:01.08 +32:54:16.1: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 16.3749* 17 12 01.08 +32 54 16.1 12.6 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,2461237.8749,12.62,0.05,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 20260716.3749 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.09 17:11:14.18 +33:14:12.5
56.23089 34.41022 galactic Her Second-epoch detections are separated by 0.4" and 4.5 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 | 17:11:14.18 +33:14:12.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.368+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:14.18 +33:14:12.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:14.18 +33:14:12.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 14.18 +33 14 12.5 12.1 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
target,2461237.8749,12.09,0.05,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 20260716.3749 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.35 17:04:16.52 +33:28:27.0
56.15212 35.88163 galactic Her Second-epoch detections are separated by 1.1" and 4.7 pix
The object was found in VSX 1" Gaia DR3 1337626817986533504
Type: RS
# Max. Min./Amp. JD0 Period
12.970 G 13.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:16.52 +33:28:27.0: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:16.52 +33:28:27.0: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 04 16.52 +33 28 27.0 12.3 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
Gaia DR3 1337626817986533504,2461237.8749,12.35,0.05,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
Gaia DR3 1337626817986533504 20260716.3749 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.62 17:11:22.77 +33:21:21.4
56.37969 34.40616 galactic Her Second-epoch detections are separated by 1.3" and 4.5 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 | 17:11:22.77 +33:21:21.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.342+/-0.032 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:22.77 +33:21:21.4: 13.78 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:22.77 +33:21:21.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 16.3749* 17 11 22.77 +33 21 21.4 12.6 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,2461237.8749,12.62,0.05,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 20260716.3749 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.07 17:10:49.35 +33:23:53.6
56.40020 34.52873 galactic Her Second-epoch detections are separated by 2.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:10:49.35 +33:23:53.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.644+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:49.35 +33:23:53.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:49.35 +33:23:53.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 16.3749* 17 10 49.35 +33 23 53.6 12.1 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
target,2461237.8749,12.07,0.05,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 20260716.3749 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.10 17:12:39.43 +33:08:00.9
56.18579 34.09774 galactic Her Second-epoch detections are separated by 0.5" and 4.4 pix
The object was found in VSX 0" V1047 Her
Type: EW
# Max. Min./Amp. JD0 Period
12.260 w 12.780 w 2452500.26400 0.320737330000 K1
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:39.43 +33:08:00.9: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:39.43 +33:08:00.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 12 39.43 +33 08 00.9 12.1 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
V1047 Her,2461237.8749,12.10,0.05,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
V1047 Her 20260716.3749 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.74 17:11:00.01 +33:39:18.1
56.71448 34.54593 galactic Her Second-epoch detections are separated by 1.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:11:00.01 +33:39:18.1 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.029 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:00.01 +33:39:18.1: 14.19 +/- 0.06 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:00.01 +33:39:18.1: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 00.01 +33 39 18.1 12.7 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,2461237.8749,12.74,0.05,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
target 20260716.3749 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.38 17:09:24.98 +29:35:16.5
51.83080 33.94510 galactic Her Second-epoch detections are separated by 1.0" and 4.5 pix
The object was found in VSX 1" Gaia DR3 1308972479815435776
Type: ROT
# Max. Min./Amp. JD0 Period
13.220 G 13.280 G G
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:24.98 +29:35:16.5: 13.39 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:24.98 +29:35:16.5: 13.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 24.98 +29 35 16.5 12.4 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 1308972479815435776,2461237.8749,12.38,0.05,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 1308972479815435776 20260716.3749 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.10 17:06:16.16 +33:31:06.0
56.30672 35.48289 galactic Her Second-epoch detections are separated by 1.6" and 4.7 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 | ATO J256.5671+33.5185 | 17:06:17.64 +33:30:46.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.942+/-0.027 (M)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:16.16 +33:31:06.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:16.16 +33:31:06.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 16.3749* 17 06 16.16 +33 31 06.0 12.1 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
ATO J256.5671+33.5185,2461237.8749,12.10,0.05,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
ATO J256.5671+33.5185 20260716.3749 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.53 17:11:45.53 +32:56:29.7
55.91007 34.24011 galactic Her Second-epoch detections are separated by 1.6" and 4.7 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 | 17:11:45.53 +32:56:29.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.527+/-0.030 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:45.53 +32:56:29.7: 14.03 +/- 0.05 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:45.53 +32:56:29.7: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 16.3749* 17 11 45.53 +32 56 29.7 12.5 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,2461237.8749,12.53,0.05,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 20260716.3749 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.65 17:07:18.37 +33:14:52.7
56.03572 35.21627 galactic Her Second-epoch detections are separated by 0.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1334594708514346240 | 17:07:18.35 +33:14:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.310+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:18.37 +33:14:52.7: 12.57 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:18.37 +33:14:52.7: 12.56 +/- 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 16.3749* 17 07 18.37 +33 14 52.7 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 1334594708514346240,2461237.8749,11.65,0.05,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 1334594708514346240 20260716.3749 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 16.3749 2461237.8749 12.42 17:08:25.97 +29:39:38.7
51.85177 34.17024 galactic Her Second-epoch detections are separated by 1.4" and 4.6 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 | 17:08:25.97 +29:39:38.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.405+/-0.026 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:25.97 +29:39:38.7: 13.45 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:25.97 +29:39:38.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 25.97 +29 39 38.7 12.4 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,2461237.8749,12.42,0.05,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 20260716.3749 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.97 17:12:28.03 +33:05:40.4
56.12939 34.12817 galactic Her Second-epoch detections are separated by 0.8" and 4.5 pix
The object was found in VSX 5" Gaia DR3 1334451153527655296
Type: ROT
# Max. Min./Amp. JD0 Period
15.160 G 15.180 G K
ATTENTION: measured mag 11.97 is 3.2 mag brighter than the VSX record maximum brightness 15.16 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:28.03 +33:05:40.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:28.03 +33:05:40.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 16.3749* 17 12 28.03 +33 05 40.4 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
Gaia DR3 1334451153527655296,2461237.8749,11.97,0.05,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
Gaia DR3 1334451153527655296 20260716.3749 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 16.3749 2461237.8749 11.97 17:12:19.66 +33:00:20.6
56.01698 34.13751 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 | 17:12:19.66 +33:00:20.6 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.031 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:19.66 +33:00:20.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:19.66 +33:00:20.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 16.3749* 17 12 19.66 +33 00 20.6 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,2461237.8749,11.97,0.05,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 20260716.3749 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 16.3749 2461237.8749 11.94 17:08:47.49 +30:47:13.1
53.19686 34.36717 galactic Her Second-epoch detections are separated by 0.9" and 4.5 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 | 17:08:47.49 +30:47:13.1 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.029 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:47.49 +30:47:13.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:47.49 +30:47:13.1: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 16.3749* 17 08 47.49 +30 47 13.1 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,2461237.8749,11.94,0.05,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
target 20260716.3749 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.96 17:05:24.43 +33:25:56.7
56.15919 35.64195 galactic Her Second-epoch detections are separated by 0.9" and 4.6 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 | Large-amplitude variable Gaia DR2 1337611665340381696 | 17:05:24.43 +33:25:56.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G7 (LAMOST DR5) J-Ks=0.539+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:24.43 +33:25:56.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:24.43 +33:25:56.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 16.3749* 17 05 24.43 +33 25 56.7 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
Large-amplitude variable Gaia DR2 1337611665340381696,2461237.8749,11.96,0.05,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 1337611665340381696 20260716.3749 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.98 17:05:09.09 +33:26:06.4
56.14940 35.69476 galactic Her Second-epoch detections are separated by 0.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J256.2839+33.4303 | 17:05:09.09 +33:26:06.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:09.09 +33:26:06.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:09.09 +33:26:06.4: 12.95 +/- 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 16.3749* 17 05 09.09 +33 26 06.4 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
ATO J256.2839+33.4303,2461237.8749,11.98,0.05,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
ATO J256.2839+33.4303 20260716.3749 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 16.3749 2461237.8749 11.93 17:07:25.55 +33:24:33.5
56.23529 35.22468 galactic Her Second-epoch detections are separated by 0.4" and 4.5 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 | 17:07:25.55 +33:24:33.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.321+/-0.034 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:25.55 +33:24:33.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:25.55 +33:24:33.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 16.3749* 17 07 25.55 +33 24 33.5 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,2461237.8749,11.93,0.05,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 20260716.3749 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 16.3749 2461237.8749 12.55 17:10:27.62 +33:15:55.4
56.22324 34.57483 galactic Her Second-epoch detections are separated by 2.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:10:27.62 +33:15:55.4 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.031 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:27.62 +33:15:55.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:27.62 +33:15:55.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 16.3749* 17 10 27.62 +33 15 55.4 12.6 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,2461237.8749,12.55,0.05,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
target 20260716.3749 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.89 17:08:22.78 +30:05:37.2
52.35598 34.28756 galactic Her Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:22.78 +30:05:37.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.411+/-0.027 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:22.78 +30:05:37.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:22.78 +30:05:37.2: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 16.3749* 17 08 22.78 +30 05 37.2 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,2461237.8749,11.89,0.05,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 20260716.3749 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 12.28 17:08:32.34 +30:01:35.5
52.28733 34.23779 galactic Her Second-epoch detections are separated by 1.1" and 4.7 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 | 17:08:32.34 +30:01:35.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.684+/-0.026 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:32.34 +30:01:35.5: 13.26 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:32.34 +30:01:35.5: 13.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 32.34 +30 01 35.5 12.3 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,2461237.8749,12.28,0.05,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 20260716.3749 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.32 17:09:18.29 +30:59:26.7
53.46806 34.30798 galactic Her Second-epoch detections are separated by 1.5" and 4.5 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 | 17:09:18.29 +30:59:26.7 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:18.29 +30:59:26.7: 13.25 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:18.29 +30:59:26.7: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 18.29 +30 59 26.7 12.3 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,2461237.8749,12.32,0.05,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 20260716.3749 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.94 17:08:32.44 +30:41:57.9
53.07835 34.39890 galactic Her Second-epoch detections are separated by 0.8" and 4.6 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 | 17:08:32.44 +30:41:57.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.284+/-0.029 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:32.44 +30:41:57.9: 12.88 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:32.44 +30:41:57.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 16.3749* 17 08 32.44 +30 41 57.9 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,2461237.8749,11.94,0.05,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
target 20260716.3749 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.95 17:04:09.66 +33:31:32.2
56.20863 35.91508 galactic Her Second-epoch detections are separated by 1.6" and 4.7 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 | 17:04:09.66 +33:31:32.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.409+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:09.66 +33:31:32.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:09.66 +33:31:32.2: 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 16.3749* 17 04 09.66 +33 31 32.2 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,2461237.8749,11.95,0.05,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
target 20260716.3749 11.95CV 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 16.3749 2461237.8749 11.88 17:05:36.63 +33:25:16.0
56.15596 35.59812 galactic Her Second-epoch detections are separated by 1.3" and 4.6 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 | 17:05:36.63 +33:25:16.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.393+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:36.63 +33:25:16.0: 12.86 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:36.63 +33:25:16.0: 12.82 +/- 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 16.3749* 17 05 36.63 +33 25 16.0 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,2461237.8749,11.88,0.05,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 20260716.3749 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 16.3749 2461237.8749 12.34 17:02:09.67 +33:21:45.3
55.91020 36.29254 galactic Her Second-epoch detections are separated by 1.4" and 4.7 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 | 17:02:09.67 +33:21:45.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.570+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:02:09.67 +33:21:45.3: 13.24 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:02:09.67 +33:21:45.3: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 02 09.67 +33 21 45.3 12.3 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,2461237.8749,12.34,0.05,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 20260716.3749 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.32 17:11:57.38 +32:51:28.7
55.82224 34.18151 galactic Her Second-epoch detections are separated by 0.8" and 4.5 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 | 17:11:57.38 +32:51:28.7 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:57.38 +32:51:28.7: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:57.38 +32:51:28.7: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 16.3749* 17 11 57.38 +32 51 28.7 12.3 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,2461237.8749,12.32,0.05,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 20260716.3749 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.28 17:08:24.22 +29:44:49.6
51.95104 34.19772 galactic Her Second-epoch detections are separated by 0.8" and 4.5 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 | 17:08:24.22 +29:44:49.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.360+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:24.22 +29:44:49.6: 13.53 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:24.22 +29:44:49.6: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 16.3749* 17 08 24.22 +29 44 49.6 12.3 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,2461237.8749,12.28,0.05,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 20260716.3749 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.44 17:10:15.76 +31:06:12.2
53.65861 34.13491 galactic Her Second-epoch detections are separated by 1.0" and 4.5 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 | 17:10:15.76 +31:06:12.2 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:15.76 +31:06:12.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:15.76 +31:06:12.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 10 15.76 +31 06 12.2 12.4 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,2461237.8749,12.44,0.05,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
target 20260716.3749 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.33 17:09:05.78 +29:00:57.3
51.14274 33.86800 galactic Her Second-epoch detections are separated by 1.1" and 4.6 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 | 17:09:05.78 +29:00:57.3 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:05.78 +29:00:57.3: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:05.78 +29:00:57.3: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 05.78 +29 00 57.3 12.3 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,2461237.8749,12.33,0.05,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 20260716.3749 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.49 17:05:06.76 +33:23:58.8
56.10464 35.69566 galactic Her Second-epoch detections are separated by 1.5" and 4.7 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 | 17:05:06.76 +33:23:58.8 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.325+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:06.76 +33:23:58.8: 13.49 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:06.76 +33:23:58.8: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 16.3749* 17 05 06.76 +33 23 58.8 12.5 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,2461237.8749,12.49,0.05,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 20260716.3749 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.46 17:05:53.26 +34:10:33.7
57.08087 35.68900 galactic Her Second-epoch detections are separated by 2.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:05:53.26 +34:10:33.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:53.26 +34:10:33.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:53.26 +34:10:33.7: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 16.3749* 17 05 53.26 +34 10 33.7 12.5 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,2461237.8749,12.46,0.05,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 20260716.3749 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.99 17:04:45.60 +33:03:03.3
55.66572 35.69797 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 | 17:04:45.60 +33:03:03.3 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.278+/-0.030 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:45.60 +33:03:03.3: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:45.60 +33:03:03.3: 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 16.3749* 17 04 45.60 +33 03 03.3 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,2461237.8749,11.99,0.05,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 20260716.3749 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.22 16:47:12.06 +34:05:25.8
56.12882 39.48229 galactic Her Second-epoch detections are separated by 0.5" and 4.6 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 | 16:47:12.06 +34:05:25.8 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.056 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:12.06 +34:05:25.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:12.06 +34:05:25.8: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 16 47 12.06 +34 05 25.8 12.2 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
target,2461237.8749,12.22,0.05,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
target 20260716.3749 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.86 17:11:54.25 +33:00:21.5
55.99407 34.22426 galactic Her Second-epoch detections are separated by 0.3" and 4.5 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 | 17:11:54.25 +33:00:21.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.767+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:54.25 +33:00:21.5: 12.84 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:54.25 +33:00:21.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 54.25 +33 00 21.5 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,2461237.8749,11.86,0.05,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 20260716.3749 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 16.3749 2461237.8749 12.63 17:11:03.11 +32:50:52.9
55.76066 34.36479 galactic Her Second-epoch detections are separated by 0.7" and 4.6 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 | 17:11:03.11 +32:50:52.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:03.11 +32:50:52.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:03.11 +32:50:52.9: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 16.3749* 17 11 03.11 +32 50 52.9 12.6 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,2461237.8749,12.63,0.05,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 20260716.3749 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.31 17:12:11.85 +33:01:53.6
56.04033 34.16974 galactic Her Second-epoch detections are separated by 1.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J258.0624+33.0248 | 17:12:11.85 +33:01:53.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:11.85 +33:01:53.6: 13.45 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:11.85 +33:01:53.6: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 12 11.85 +33 01 53.6 12.3 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
ATO J258.0624+33.0248,2461237.8749,12.31,0.05,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 J258.0624+33.0248 20260716.3749 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.09 17:09:07.25 +29:48:40.8
52.07262 34.06277 galactic Her Second-epoch detections are separated by 1.5" and 4.7 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 | 17:09:07.25 +29:48:40.8 (user input) | T | P | (position from user input) J-Ks=0.857+/-0.024 (M)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:07.25 +29:48:40.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:07.25 +29:48:40.8: 13.19 +/- 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 16.3749* 17 09 07.25 +29 48 40.8 12.1 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
target,2461237.8749,12.09,0.05,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 20260716.3749 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.16 17:08:00.37 +30:12:15.5
52.46235 34.39266 galactic Her Second-epoch detections are separated by 1.0" and 4.5 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 | 17:08:00.37 +30:12:15.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.624+/-0.029 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:00.37 +30:12:15.5: 13.22 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:00.37 +30:12:15.5: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 00.37 +30 12 15.5 12.2 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
target,2461237.8749,12.16,0.05,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 20260716.3749 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.26 17:08:50.75 +30:50:48.7
53.27070 34.36993 galactic Her Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:50.75 +30:50:48.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.526+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:50.75 +30:50:48.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:50.75 +30:50:48.7: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 50.75 +30 50 48.7 12.3 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,2461237.8749,12.26,0.05,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 20260716.3749 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.07 17:05:34.31 +33:14:07.2
55.93017 35.56878 galactic Her Second-epoch detections are separated by 0.4" and 4.5 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 | 17:05:34.31 +33:14:07.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.687+/-0.029 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:34.31 +33:14:07.2: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:34.31 +33:14:07.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 16.3749* 17 05 34.31 +33 14 07.2 12.1 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
target,2461237.8749,12.07,0.05,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 20260716.3749 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.36 17:10:11.23 +33:17:09.1
56.23300 34.63495 galactic Her Second-epoch detections are separated by 1.4" and 4.5 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 | 17:10:11.23 +33:17:09.1 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:11.23 +33:17:09.1: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:11.23 +33:17:09.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 10 11.23 +33 17 09.1 12.4 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,2461237.8749,12.36,0.05,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 20260716.3749 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 12.55 17:03:59.55 +33:40:18.9
56.37747 35.97795 galactic Her Second-epoch detections are separated by 1.6" and 4.6 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 | 17:03:59.55 +33:40:18.9 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.030 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:03:59.55 +33:40:18.9: 13.67 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:03:59.55 +33:40:18.9: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 16.3749* 17 03 59.55 +33 40 18.9 12.6 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,2461237.8749,12.55,0.05,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
target 20260716.3749 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.29 17:11:24.30 +33:30:35.2
56.56337 34.43326 galactic Her Second-epoch detections are separated by 1.0" and 4.6 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 | 17:11:24.30 +33:30:35.2 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.035 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:24.30 +33:30:35.2: 13.18 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:24.30 +33:30:35.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 24.30 +33 30 35.2 12.3 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,2461237.8749,12.29,0.05,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 20260716.3749 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.27 17:04:51.71 +33:48:07.4
56.57826 35.82581 galactic Her Second-epoch detections are separated by 0.5" and 4.6 pix
The object was found in VSX 1" Gaia DR3 1337685676218334336
Type: RS
# Max. Min./Amp. JD0 Period
13.180 G 13.320 G G
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:51.71 +33:48:07.4: 13.22 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:51.71 +33:48:07.4: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 04 51.71 +33 48 07.4 12.3 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
Gaia DR3 1337685676218334336,2461237.8749,12.27,0.05,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 1337685676218334336 20260716.3749 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.63 17:09:16.92 +32:19:47.4
55.04865 34.61600 galactic Her Second-epoch detections are separated by 0.1" and 4.6 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 1334303922048752512 | 17:09:16.94 +32:19:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.437+/-0.027 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:16.92 +32:19:47.4: 12.55 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:16.92 +32:19:47.4: 12.59 +/- 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 16.3749* 17 09 16.92 +32 19 47.4 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 1334303922048752512,2461237.8749,11.63,0.05,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
Gaia DR3 1334303922048752512 20260716.3749 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 16.3749 2461237.8749 12.54 17:08:31.05 +28:44:41.8
50.78804 33.92088 galactic Her Second-epoch detections are separated by 2.5" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:31.05 +28:44:41.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.450+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:31.05 +28:44:41.8: 13.88 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:31.05 +28:44:41.8: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 16.3749* 17 08 31.05 +28 44 41.8 12.5 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,2461237.8749,12.54,0.05,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 20260716.3749 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.16 17:10:13.17 +33:24:33.7
56.38153 34.65413 galactic Her Second-epoch detections are separated by 0.8" and 4.5 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 | 17:10:13.17 +33:24:33.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.379+/-0.027 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:13.17 +33:24:33.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:13.17 +33:24:33.7: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 10 13.17 +33 24 33.7 12.2 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
target,2461237.8749,12.16,0.05,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 20260716.3749 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.72 17:11:15.57 +33:08:46.1
56.12476 34.38622 galactic Her Second-epoch detections are separated by 1.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1334460533736246144 | 17:11:15.57 +33:08:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.768+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:15.57 +33:08:46.1: 12.80 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:15.57 +33:08:46.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 16.3749* 17 11 15.57 +33 08 46.1 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 1334460533736246144,2461237.8749,11.72,0.05,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 1334460533736246144 20260716.3749 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.31 17:08:56.84 +32:23:44.8
55.10815 34.69936 galactic Her Second-epoch detections are separated by 0.3" and 4.6 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 | 17:08:56.84 +32:23:44.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.288+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:56.84 +32:23:44.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:56.84 +32:23:44.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 16.3749* 17 08 56.84 +32 23 44.8 12.3 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,2461237.8749,12.31,0.05,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 20260716.3749 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.41 17:10:57.22 +32:41:11.6
55.56430 34.34992 galactic Her Second-epoch detections are separated by 0.7" and 4.5 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 | 17:10:57.22 +32:41:11.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:57.22 +32:41:11.6: 13.41 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:57.22 +32:41:11.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 10 57.22 +32 41 11.6 12.4 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,2461237.8749,12.41,0.05,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 20260716.3749 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.83 17:07:03.59 +33:07:34.4
55.87690 35.24174 galactic Her Second-epoch detections are separated by 1.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J256.7600+33.1287 | 17:07:03.59 +33:07:34.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.674+/-0.026 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:03.59 +33:07:34.4: 12.80 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:03.59 +33:07:34.4: 12.81 +/- 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 16.3749* 17 07 03.59 +33 07 34.4 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
ATO J256.7600+33.1287,2461237.8749,11.83,0.05,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 J256.7600+33.1287 20260716.3749 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.54 17:11:46.70 +33:03:22.5
56.04660 34.26084 galactic Her Second-epoch detections are separated by 1.2" and 4.6 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 | 17:11:46.70 +33:03:22.5 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.575+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:46.70 +33:03:22.5: 13.86 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:46.70 +33:03:22.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 16.3749* 17 11 46.70 +33 03 22.5 12.5 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,2461237.8749,12.54,0.05,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 20260716.3749 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.53 17:05:17.62 +33:24:58.8
56.13400 35.66196 galactic Her Second-epoch detections are separated by 0.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:05:17.62 +33:24:58.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.256+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:17.62 +33:24:58.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:17.62 +33:24:58.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 05 17.62 +33 24 58.8 12.5 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,2461237.8749,12.53,0.05,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 20260716.3749 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.12 17:05:44.99 +33:00:31.9
55.66700 35.48628 galactic Her Second-epoch detections are separated by 0.5" and 4.6 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 | 17:05:44.99 +33:00:31.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.353+/-0.034 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:44.99 +33:00:31.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:44.99 +33:00:31.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 16.3749* 17 05 44.99 +33 00 31.9 12.1 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
target,2461237.8749,12.12,0.05,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 20260716.3749 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.14 16:47:04.36 +34:08:54.9
56.19783 39.51754 galactic Her Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:47:04.36 +34:08:54.9 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.032 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:04.36 +34:08:54.9: 13.15 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:04.36 +34:08:54.9: 13.09 +/- 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 16.3749* 16 47 04.36 +34 08 54.9 12.1 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
target,2461237.8749,12.14,0.05,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 20260716.3749 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.12 17:08:25.39 +30:41:12.9
53.05640 34.42049 galactic Her Second-epoch detections are separated by 0.3" and 4.6 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 | 17:08:25.39 +30:41:12.9 (user input) | T | P | (position from user input) J-Ks=0.524+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:25.39 +30:41:12.9: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:25.39 +30:41:12.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 16.3749* 17 08 25.39 +30 41 12.9 12.1 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
target,2461237.8749,12.12,0.05,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 20260716.3749 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.08 17:11:43.70 +33:16:07.8
56.29524 34.31649 galactic Her Second-epoch detections are separated by 0.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:11:43.70 +33:16:07.8 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.580+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:43.70 +33:16:07.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:43.70 +33:16:07.8: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 43.70 +33 16 07.8 12.1 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
target,2461237.8749,12.08,0.05,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 20260716.3749 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 12.11 17:05:01.01 +33:32:19.0
56.26752 35.74275 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 | 17:05:01.01 +33:32:19.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.532+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:01.01 +33:32:19.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:01.01 +33:32:19.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 16.3749* 17 05 01.01 +33 32 19.0 12.1 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
target,2461237.8749,12.11,0.05,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 20260716.3749 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.57 17:04:58.22 +33:29:38.1
56.21118 35.74344 galactic Her Second-epoch detections are separated by 0.3" and 4.5 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 | 17:04:58.22 +33:29:38.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.545+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:58.22 +33:29:38.1: 13.65 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:58.22 +33:29:38.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 16.3749* 17 04 58.22 +33 29 38.1 12.6 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,2461237.8749,12.57,0.05,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
target 20260716.3749 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.02 17:12:06.93 +33:13:21.4
56.26147 34.22755 galactic Her Second-epoch detections are separated by 0.5" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:12:06.93 +33:13:21.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.532+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:06.93 +33:13:21.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:06.93 +33:13:21.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 16.3749* 17 12 06.93 +33 13 21.4 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,2461237.8749,12.02,0.05,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 20260716.3749 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 12.34 17:08:34.43 +29:51:55.1
52.10053 34.19103 galactic Her Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:34.43 +29:51:55.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.406+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:34.43 +29:51:55.1: 13.41 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:34.43 +29:51:55.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 34.43 +29 51 55.1 12.3 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,2461237.8749,12.34,0.05,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 20260716.3749 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.49 17:06:32.02 +33:18:42.1
56.07189 35.38732 galactic Her Second-epoch detections are separated by 0.1" and 4.5 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 1334606936284556160 | 17:06:32.03 +33:18:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.293+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:32.02 +33:18:42.1: 12.46 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:32.02 +33:18:42.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 16.3749* 17 06 32.02 +33 18 42.1 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
Gaia DR3 1334606936284556160,2461237.8749,11.49,0.05,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 1334606936284556160 20260716.3749 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.56 17:05:59.49 +33:48:36.2
56.64414 35.59718 galactic Her Second-epoch detections are separated by 1.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J256.5092+33.8079 | 17:05:59.49 +33:48:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.410+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:59.49 +33:48:36.2: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:59.49 +33:48:36.2: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 16.3749* 17 05 59.49 +33 48 36.2 12.6 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
ATO J256.5092+33.8079,2461237.8749,12.56,0.05,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
ATO J256.5092+33.8079 20260716.3749 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.20 17:08:18.90 +30:41:27.7
53.05459 34.44406 galactic Her Second-epoch detections are separated by 0.3" and 4.6 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 | 17:08:18.90 +30:41:27.7 (user input) | T | P | (position from user input) J-Ks=0.695+/-0.026 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:18.90 +30:41:27.7: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:18.90 +30:41:27.7: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 16.3749* 17 08 18.90 +30 41 27.7 12.2 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
target,2461237.8749,12.20,0.05,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 20260716.3749 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.71 16:49:11.27 +34:05:49.8
56.22113 39.07715 galactic Her Second-epoch detections are separated by 5.2" and 4.7 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 | Large-amplitude variable Gaia DR2 1314802399702576000 | 16:49:11.27 +34:05:49.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.336+/-0.035 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:49:11.27 +34:05:49.8: 13.81 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:49:11.27 +34:05:49.8: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 16.3749* 16 49 11.27 +34 05 49.8 12.7 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
Large-amplitude variable Gaia DR2 1314802399702576000,2461237.8749,12.71,0.05,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 1314802399702576000 20260716.3749 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.47 17:07:11.02 +29:58:39.1
52.14336 34.51052 galactic Her Second-epoch detections are separated by 3.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1309195027839948800 | 17:07:14.01 +29:58:40.1 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.435+/-0.031 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:11.02 +29:58:39.1: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:11.02 +29:58:39.1: 13.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 16.3749* 17 07 11.02 +29 58 39.1 12.5 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
Gaia DR3 1309195027839948800,2461237.8749,12.47,0.05,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 1309195027839948800 20260716.3749 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.05 17:09:24.82 +30:44:45.5
53.18686 34.22762 galactic Her Second-epoch detections are separated by 1.0" and 4.6 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 1309386647804589568 | 17:09:26.82 +30:44:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.638+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:24.82 +30:44:45.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:24.82 +30:44:45.5: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 16.3749* 17 09 24.82 +30 44 45.5 12.1 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 1309386647804589568,2461237.8749,12.05,0.05,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 1309386647804589568 20260716.3749 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.21 17:04:54.56 +33:01:16.8
55.63786 35.66132 galactic Her Second-epoch detections are separated by 1.3" and 4.6 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 | 17:04:54.56 +33:01:16.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.534+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:54.56 +33:01:16.8: 13.08 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:54.56 +33:01:16.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 16.3749* 17 04 54.56 +33 01 16.8 12.2 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
target,2461237.8749,12.21,0.05,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
target 20260716.3749 12.21CV 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 16.3749 2461237.8749 11.42 17:11:40.59 +32:53:35.0
55.84823 34.24648 galactic Her Second-epoch detections are separated by 0.5" and 4.5 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 1334418851077535232 | 17:11:40.64 +32:53:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:40.59 +32:53:35.0: 12.42 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:40.59 +32:53:35.0: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 16.3749* 17 11 40.59 +32 53 35.0 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 1334418851077535232,2461237.8749,11.42,0.05,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 1334418851077535232 20260716.3749 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.31 17:08:58.11 +30:45:51.3
53.18097 34.32487 galactic Her Second-epoch detections are separated by 1.0" and 4.5 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 | 17:08:58.11 +30:45:51.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:58.11 +30:45:51.3: 13.39 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:58.11 +30:45:51.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 16.3749* 17 08 58.11 +30 45 51.3 12.3 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,2461237.8749,12.31,0.05,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 20260716.3749 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.10 17:08:30.39 +30:46:17.1
53.16107 34.42300 galactic Her Second-epoch detections are separated by 1.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J257.1239+30.7670 | 17:08:30.39 +30:46:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.684+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:30.39 +30:46:17.1: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:30.39 +30:46:17.1: 13.13 +/- 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 16.3749* 17 08 30.39 +30 46 17.1 12.1 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
ATO J257.1239+30.7670,2461237.8749,12.10,0.05,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
ATO J257.1239+30.7670 20260716.3749 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.36 16:46:29.13 +34:11:02.0
56.21884 39.64299 galactic Her Second-epoch detections are separated by 2.3" and 4.5 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 | 16:46:29.13 +34:11:02.0 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.032 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:46:29.13 +34:11:02.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:46:29.13 +34:11:02.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 16.3749* 16 46 29.13 +34 11 02.0 12.4 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,2461237.8749,12.36,0.05,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 20260716.3749 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 11.49 17:06:55.29 +33:04:25.0
55.80655 35.25926 galactic Her Second-epoch detections are separated by 1.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1334591611841250304 | 17:06:55.32 +33:04:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:55.29 +33:04:25.0: 12.39 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:55.29 +33:04:25.0: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 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 16.3749* 17 06 55.29 +33 04 25.0 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
Gaia DR3 1334591611841250304,2461237.8749,11.49,0.05,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 1334591611841250304 20260716.3749 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 10.87 17:06:30.81 +33:17:46.4
56.05226 35.38831 galactic Her Second-epoch detections are separated by 0.3" and 4.5 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 1334606768782529664 | 17:06:30.81 +33:17:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.683+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:30.81 +33:17:46.4: 11.72 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:30.81 +33:17:46.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 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 16.3749* 17 06 30.81 +33 17 46.4 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 1334606768782529664,2461237.8749,10.87,0.05,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 1334606768782529664 20260716.3749 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.39 17:07:10.85 +33:19:39.7
56.12473 35.25818 galactic Her Second-epoch detections are separated by 0.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1334607692198799872 | 17:07:10.83 +33:19:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.601+/-0.026 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:10.85 +33:19:39.7: 12.36 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:10.85 +33:19:39.7: 12.31 +/- 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 16.3749* 17 07 10.85 +33 19 39.7 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 1334607692198799872,2461237.8749,11.39,0.05,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
Gaia DR3 1334607692198799872 20260716.3749 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 16.3749 2461237.8749 11.46 17:09:27.77 +29:13:06.2
51.40306 33.84220 galactic Her Second-epoch detections are separated by 0.2" and 4.6 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 | Large-amplitude variable Gaia DR2 1308892455984124544 | 17:09:27.79 +29:13:06.3 (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=0.458+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:27.77 +29:13:06.2: 12.35 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:27.77 +29:13:06.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 27.77 +29 13 06.2 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
Large-amplitude variable Gaia DR2 1308892455984124544,2461237.8749,11.46,0.05,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 1308892455984124544 20260716.3749 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.39 17:11:43.56 +33:05:11.4
56.07950 34.27804 galactic Her Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1334456268832747392 | 17:11:43.53 +33:05:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:43.56 +33:05:11.4: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:43.56 +33:05:11.4: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 16.3749* 17 11 43.56 +33 05 11.4 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
Gaia DR3 1334456268832747392,2461237.8749,11.39,0.05,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
Gaia DR3 1334456268832747392 20260716.3749 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 16.3749 2461237.8749 12.22 17:11:25.83 +33:15:13.4
56.26135 34.37413 galactic Her Second-epoch detections are separated by 1.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:11:25.83 +33:15:13.4 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:25.83 +33:15:13.4: 13.36 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:25.83 +33:15:13.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 25.83 +33 15 13.4 12.2 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
target,2461237.8749,12.22,0.05,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
target 20260716.3749 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.46 17:04:46.11 +33:54:06.9
56.69454 35.86407 galactic Her Second-epoch detections are separated by 1.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:04:46.11 +33:54:06.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.376+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:46.11 +33:54:06.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:46.11 +33:54:06.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 16.3749* 17 04 46.11 +33 54 06.9 12.5 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,2461237.8749,12.46,0.05,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 20260716.3749 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.33 17:07:33.52 +30:04:40.2
52.28526 34.45603 galactic Her Second-epoch detections are separated by 1.1" and 4.5 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 | 17:07:33.52 +30:04:40.2 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:33.52 +30:04:40.2: 13.36 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:33.52 +30:04:40.2: 13.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 07 33.52 +30 04 40.2 12.3 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,2461237.8749,12.33,0.05,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 20260716.3749 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.59 17:04:57.60 +33:19:49.2
56.01315 35.71310 galactic Her Second-epoch detections are separated by 1.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:04:57.60 +33:19:49.2 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:57.60 +33:19:49.2: 13.82 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:57.60 +33:19:49.2: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 16.3749* 17 04 57.60 +33 19 49.2 12.6 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,2461237.8749,12.59,0.05,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 20260716.3749 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.54 17:07:44.43 +30:04:19.6
52.29006 34.41648 galactic Her Second-epoch detections are separated by 1.7" and 4.6 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 | 17:07:44.43 +30:04:19.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.690+/-0.030 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:44.43 +30:04:19.6: 13.79 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:44.43 +30:04:19.6: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 16.3749* 17 07 44.43 +30 04 19.6 12.5 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,2461237.8749,12.54,0.05,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 20260716.3749 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.40 17:09:41.79 +33:17:50.4
56.22059 34.73762 galactic Her Second-epoch detections are separated by 0.5" and 4.6 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 | 17:09:41.79 +33:17:50.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.559+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:41.79 +33:17:50.4: 13.35 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:41.79 +33:17:50.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 41.79 +33 17 50.4 12.4 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,2461237.8749,12.40,0.05,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 20260716.3749 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.24 17:12:13.94 +33:03:51.5
56.08088 34.16968 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 | 17:12:13.94 +33:03:51.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:13.94 +33:03:51.5: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:13.94 +33:03:51.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 12 13.94 +33 03 51.5 12.2 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
target,2461237.8749,12.24,0.05,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 20260716.3749 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.71 17:12:08.08 +33:06:06.5
56.11982 34.19774 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 | 17:12:08.08 +33:06:06.5 (user input) | T | P | (position from user input) J-Ks=0.523+/-0.030 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:08.08 +33:06:06.5: 12.74 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:08.08 +33:06:06.5: 12.78 +/- 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 16.3749* 17 12 08.08 +33 06 06.5 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,2461237.8749,11.71,0.05,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 20260716.3749 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.29 17:09:00.51 +28:58:38.0
51.09177 33.87667 galactic Her Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1308880086478287872 | 17:09:00.48 +28:58:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.325+/-0.026 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:00.51 +28:58:38.0: 12.30 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:00.51 +28:58:38.0: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 16.3749* 17 09 00.51 +28 58 38.0 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
Gaia DR3 1308880086478287872,2461237.8749,11.29,0.05,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 1308880086478287872 20260716.3749 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.29 17:04:18.97 +33:36:25.8
56.31517 35.89930 galactic Her Second-epoch detections are separated by 0.9" and 4.6 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 | 17:04:18.97 +33:36:25.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.352+/-0.051 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:18.97 +33:36:25.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:18.97 +33:36:25.8: 13.27 +/- 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 16.3749* 17 04 18.97 +33 36 25.8 12.3 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,2461237.8749,12.29,0.05,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 20260716.3749 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.12 17:05:01.17 +33:37:55.5
56.38059 35.76056 galactic Her Second-epoch detections are separated by 0.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:05:01.17 +33:37:55.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.396+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:01.17 +33:37:55.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:01.17 +33:37:55.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 16.3749* 17 05 01.17 +33 37 55.5 12.1 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
target,2461237.8749,12.12,0.05,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 20260716.3749 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.31 16:47:14.08 +33:57:01.5
55.95102 39.45343 galactic Her Second-epoch detections are separated by 2.0" and 4.6 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 | 16:47:14.08 +33:57:01.5 (user input) | T | P | (position from user input) SpType: em 1994AJ....108..268B BPS BS 16552- 14 J-Ks=0.954+/-0.029 (M)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:14.08 +33:57:01.5: 13.33 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:14.08 +33:57:01.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 16 47 14.08 +33 57 01.5 12.3 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,2461237.8749,12.31,0.05,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 20260716.3749 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.81 17:12:51.96 +33:08:50.5
56.21342 34.05803 galactic Her Second-epoch detections are separated by 1.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J258.2164+33.1475 | 17:12:51.96 +33:08:50.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.319+/-0.030 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:51.96 +33:08:50.5: 12.71 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:51.96 +33:08:50.5: 12.75 +/- 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 16.3749* 17 12 51.96 +33 08 50.5 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
ATO J258.2164+33.1475,2461237.8749,11.81,0.05,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 J258.2164+33.1475 20260716.3749 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.66 17:11:06.02 +32:55:02.9
55.84547 34.36983 galactic Her Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:11:06.02 +32:55:02.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.379+/-0.027 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:06.02 +32:55:02.9: 12.72 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:06.02 +32:55:02.9: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 06.02 +32 55 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
target,2461237.8749,11.66,0.05,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 20260716.3749 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.07 17:09:44.12 +29:26:08.0
51.67411 33.83969 galactic Her Second-epoch detections are separated by 0.8" and 4.7 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 | 17:09:44.12 +29:26:08.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.376+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:44.12 +29:26:08.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:44.12 +29:26:08.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 16.3749* 17 09 44.12 +29 26 08.0 12.1 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
target,2461237.8749,12.07,0.05,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 20260716.3749 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.34 16:45:39.59 +33:23:43.6
55.17226 39.68792 galactic Her Second-epoch detections are separated by 1.8" and 4.7 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 | 16:45:39.59 +33:23:43.6 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.029 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:45:39.59 +33:23:43.6: 13.33 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:45:39.59 +33:23:43.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 16 45 39.59 +33 23 43.6 12.3 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,2461237.8749,12.34,0.05,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 20260716.3749 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.69 17:09:35.66 +29:01:03.1
51.17817 33.76317 galactic Her Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:09:35.66 +29:01:03.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.433+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:35.66 +29:01:03.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:35.66 +29:01:03.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 09 35.66 +29 01 03.1 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,2461237.8749,11.69,0.05,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 20260716.3749 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 16.3749 2461237.8749 11.38 17:07:06.02 +33:17:01.5
56.06784 35.26570 galactic Her Second-epoch detections are separated by 0.1" and 4.5 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 1334595430068858112 | 17:07:06.03 +33:17:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.338+/-0.026 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:06.02 +33:17:01.5: 12.26 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:06.02 +33:17:01.5: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 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 16.3749* 17 07 06.02 +33 17 01.5 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 1334595430068858112,2461237.8749,11.38,0.05,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 1334595430068858112 20260716.3749 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.24 17:06:54.15 +33:12:37.1
55.96943 35.29120 galactic Her Second-epoch detections are separated by 1.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:06:54.15 +33:12:37.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.430+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:54.15 +33:12:37.1: 13.32 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:54.15 +33:12:37.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 06 54.15 +33 12 37.1 12.2 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
target,2461237.8749,12.24,0.05,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 20260716.3749 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 10.70 17:06:42.56 +33:07:19.6
55.85351 35.31272 galactic Her Second-epoch detections are separated by 0.2" and 4.5 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 1334592715649522560 | 17:06:42.55 +33:07:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.274+/-0.028 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:42.56 +33:07:19.6: 11.53 +/- 0.00 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:42.56 +33:07:19.6: 11.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.53 +/- 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 16.3749* 17 06 42.56 +33 07 19.6 10.7 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 1334592715649522560,2461237.8749,10.70,0.05,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 1334592715649522560 20260716.3749 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.29 17:11:28.51 +33:09:44.5
56.15562 34.34557 galactic Her Second-epoch detections are separated by 1.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:11:28.51 +33:09:44.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.729+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:28.51 +33:09:44.5: 13.54 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:28.51 +33:09:44.5: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 28.51 +33 09 44.5 12.3 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,2461237.8749,12.29,0.05,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 20260716.3749 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.49 17:06:58.12 +30:01:17.6
52.18156 34.56633 galactic Her Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:06:58.12 +30:01:17.6 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.031 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:58.12 +30:01:17.6: 13.78 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:58.12 +30:01:17.6: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 16.3749* 17 06 58.12 +30 01 17.6 12.5 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,2461237.8749,12.49,0.05,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 20260716.3749 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.12 17:05:03.04 +32:57:29.9
55.56935 35.61948 galactic Her Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:05:03.04 +32:57:29.9 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.561+/-0.026 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:03.04 +32:57:29.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:03.04 +32:57:29.9: 12.99 +/- 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 16.3749* 17 05 03.04 +32 57 29.9 12.1 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
target,2461237.8749,12.12,0.05,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 20260716.3749 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.22 17:06:52.50 +30:01:20.3
52.17650 34.58619 galactic Her Second-epoch detections are separated by 1.3" and 4.5 pix
The object was found in VSX25" Gaia DR3 1309199047929363072
Type: ROT
# Max. Min./Amp. JD0 Period
13.490 G 13.510 G K
The object was not found in astcheck.
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:52.50 +30:01:20.3: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:52.50 +30:01:20.3: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 06 52.50 +30 01 20.3 12.2 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 1309199047929363072,2461237.8749,12.22,0.05,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
Gaia DR3 1309199047929363072 20260716.3749 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.40 17:08:26.43 +32:52:03.2
55.64149 34.90470 galactic Her Second-epoch detections are separated by 1.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:26.43 +32:52:03.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.813+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:26.43 +32:52:03.2: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:26.43 +32:52:03.2: 13.31 +/- 0.02 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 16.3749* 17 08 26.43 +32 52 03.2 12.4 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,2461237.8749,12.40,0.05,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 20260716.3749 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.70 17:08:52.59 +29:00:53.4
51.12668 33.91419 galactic Her Second-epoch detections are separated by 0.9" and 4.6 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 1308880430075682432 | 17:08:52.61 +29:00:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:52.59 +29:00:53.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:52.59 +29:00:53.4: 12.75 +/- 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 16.3749* 17 08 52.59 +29 00 53.4 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 1308880430075682432,2461237.8749,11.70,0.05,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 1308880430075682432 20260716.3749 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.23 17:08:45.76 +28:57:14.7
51.04824 33.92272 galactic Her Second-epoch detections are separated by 0.0" and 4.7 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 1308879811600386304 | 17:08:45.87 +28:57:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:45.76 +28:57:14.7: 12.21 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:45.76 +28:57:14.7: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 16.3749* 17 08 45.76 +28 57 14.7 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 1308879811600386304,2461237.8749,11.23,0.05,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 1308879811600386304 20260716.3749 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.41 17:05:58.77 +33:18:36.1
56.04118 35.50037 galactic Her Second-epoch detections are separated by 1.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:05:58.77 +33:18:36.1 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.299+/-0.030 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:58.77 +33:18:36.1: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:58.77 +33:18:36.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 16.3749* 17 05 58.77 +33 18 36.1 12.4 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,2461237.8749,12.41,0.05,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 20260716.3749 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.50 17:11:56.32 +33:04:28.0
56.07683 34.23195 galactic Her Second-epoch detections are separated by 0.8" and 4.5 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 | 17:11:56.32 +33:04:28.0 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.651+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:56.32 +33:04:28.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:56.32 +33:04:28.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 16.3749* 17 11 56.32 +33 04 28.0 12.5 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,2461237.8749,12.50,0.05,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 20260716.3749 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.70 17:05:09.06 +33:40:36.0
56.44106 35.74245 galactic Her Second-epoch detections are separated by 0.9" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1337632830940626688 | 17:05:09.05 +33:40:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.415+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:09.06 +33:40:36.0: 12.66 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:09.06 +33:40:36.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 05 09.06 +33 40 36.0 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 1337632830940626688,2461237.8749,11.70,0.05,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 1337632830940626688 20260716.3749 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.37 17:06:52.54 +33:02:08.3
55.75862 35.26083 galactic Her Second-epoch detections are separated by 2.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:06:52.54 +33:02:08.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.322+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:52.54 +33:02:08.3: 13.74 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:52.54 +33:02:08.3: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 16.3749* 17 06 52.54 +33 02 08.3 12.4 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,2461237.8749,12.37,0.05,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
target 20260716.3749 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.93 17:09:11.81 +32:29:34.4
55.23733 34.66906 galactic Her Second-epoch detections are separated by 0.4" and 4.5 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 | 17:09:11.81 +32:29:34.4 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.029 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:11.81 +32:29:34.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:11.81 +32:29:34.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 16.3749* 17 09 11.81 +32 29 34.4 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,2461237.8749,11.93,0.05,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 20260716.3749 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 16.3749 2461237.8749 12.58 17:04:06.59 +33:35:50.0
56.29280 35.93950 galactic Her Second-epoch detections are separated by 3.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:04:06.59 +33:35:50.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.433+/-0.029 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:06.59 +33:35:50.0: 13.91 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:06.59 +33:35:50.0: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 16.3749* 17 04 06.59 +33 35 50.0 12.6 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,2461237.8749,12.58,0.05,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
target 20260716.3749 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.24 17:06:01.39 +33:20:25.7
56.08007 35.49757 galactic Her Second-epoch detections are separated by 1.5" and 4.7 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 | 17:06:01.39 +33:20:25.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.363+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:01.39 +33:20:25.7: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:01.39 +33:20:25.7: 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 16.3749* 17 06 01.39 +33 20 25.7 12.2 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
target,2461237.8749,12.24,0.05,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 20260716.3749 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.02 17:06:17.78 +33:31:35.9
56.31810 35.47903 galactic Her Second-epoch detections are separated by 1.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J256.5671+33.5185 | 17:06:17.78 +33:31:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.589+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:17.78 +33:31:35.9: 13.00 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:17.78 +33:31:35.9: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 16.3749* 17 06 17.78 +33 31 35.9 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
ATO J256.5671+33.5185,2461237.8749,12.02,0.05,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 J256.5671+33.5185 20260716.3749 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 16.3749 2461237.8749 12.46 17:08:04.90 +29:28:13.4
51.60594 34.19691 galactic Her Second-epoch detections are separated by 1.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:08:04.90 +29:28:13.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.485+/-0.032 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:04.90 +29:28:13.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:04.90 +29:28:13.4: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 16.3749* 17 08 04.90 +29 28 13.4 12.5 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,2461237.8749,12.46,0.05,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 20260716.3749 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.51 17:08:51.14 +28:50:33.5
50.92453 33.87516 galactic Her Second-epoch detections are separated by 2.0" and 4.5 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 | 17:08:51.14 +28:50:33.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.370+/-0.028 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:51.14 +28:50:33.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:51.14 +28:50:33.5: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 16.3749* 17 08 51.14 +28 50 33.5 12.5 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,2461237.8749,12.51,0.05,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 20260716.3749 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.96 16:47:24.01 +34:06:33.3
56.16113 39.44448 galactic Her Second-epoch detections are separated by 0.7" and 4.6 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 | 16:47:24.01 +34:06:33.3 (user input) | T | P | (position from user input) J-Ks=0.583+/-0.031 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:24.01 +34:06:33.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:24.01 +34:06:33.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 16.3749* 16 47 24.01 +34 06 33.3 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,2461237.8749,11.96,0.05,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 20260716.3749 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.38 17:02:20.65 +33:06:43.1
55.61472 36.20601 galactic Her Second-epoch detections are separated by 0.6" and 4.6 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 | 17:02:20.65 +33:06:43.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.400+/-0.031 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:02:20.65 +33:06:43.1: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:02:20.65 +33:06:43.1: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 02 20.65 +33 06 43.1 12.4 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,2461237.8749,12.38,0.05,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 20260716.3749 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.23 17:11:18.92 +33:09:56.5
56.15093 34.37896 galactic Her Second-epoch detections are separated by 0.7" and 4.5 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 | 17:11:18.92 +33:09:56.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.499+/-0.027 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:18.92 +33:09:56.5: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:18.92 +33:09:56.5: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 16.3749* 17 11 18.92 +33 09 56.5 12.2 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
target,2461237.8749,12.23,0.05,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 20260716.3749 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 11.48 17:08:49.14 +28:53:39.8
50.98252 33.89551 galactic Her Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J257.2046+28.8945 | 17:08:49.11 +28:53:40.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.314+/-0.027 (F)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:49.14 +28:53:39.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:49.14 +28:53:39.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 08 49.14 +28 53 39.8 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
ATO J257.2046+28.8945,2461237.8749,11.48,0.05,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
ATO J257.2046+28.8945 20260716.3749 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 16.3749 2461237.8749 12.39 17:11:33.99 +33:36:56.4
56.69743 34.42245 galactic Her Second-epoch detections are separated by 1.6" and 4.5 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 | 17:11:33.99 +33:36:56.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:33.99 +33:36:56.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:33.99 +33:36:56.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3749* 17 11 33.99 +33 36 56.4 12.4 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,2461237.8749,12.39,0.05,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
target 20260716.3749 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3749 2461237.8749 12.38 17:08:43.44 +30:13:57.1
52.54082 34.24898 galactic Her Second-epoch detections are separated by 1.1" and 4.5 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 | 17:08:43.44 +30:13:57.1 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.028 (K)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:43.44 +30:13:57.1: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:43.44 +30:13:57.1: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 16.3749* 17 08 43.44 +30 13 57.1 12.4 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,2461237.8749,12.38,0.05,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 20260716.3749 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461172.86518891 12.05.2026 08:45:42.322 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
First image: 2461172.86518891 12.05.2026 08:45:42.322 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Last image: 2461237.87515135 16.07.2026 09:00:03.077 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 6 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): 9739
Objects passed selection criteria: 9664
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: 5772.5
Average stars matched: 5735.25 (99.3547 %)
Memory usage VmPeak: 119592 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:12:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461172.86518891 12.05.2026 08:45:42.322 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
First image: 2461172.86518891 12.05.2026 08:45:42.322 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Last image: 2461237.87515135 16.07.2026 09:00:03.077 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 236
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 59488
Objects passed selection criteria: 59254
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: 36923.2
Average stars matched: 35648.5 (96.5476 %)
Memory usage VmPeak: 166768 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:15:16 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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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: 2461237.87467166
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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits exists and is non-empty
Saving wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits to local_wcs_cache/
'wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits' -> 'local_wcs_cache/wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits'
wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits exists and is non-empty
Saving wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits to local_wcs_cache/
'wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits' -> 'local_wcs_cache/wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits'
wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits exists and is non-empty
Saving wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits to local_wcs_cache/
'wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits' -> 'local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits'
wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits exists and is non-empty
Saving wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits to local_wcs_cache/
'wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits' -> 'local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits (1st reference image)
verification OK: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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: 17:00:01.882 +29:59:45.68 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-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Image size: 937.5'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: 16:59:51.823 +29:58:47.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:00:01.882 +29:59:45.68
Second-epoch image center 16:59:51.823 +29:58:47.11
Angular distance between the image centers 0.0398 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Image size: 937.5'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: 16:59:53.416 +29:58:28.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:00:01.882 +29:59:45.68
Second-epoch image center 16:59:53.416 +29:58:28.22
Angular distance between the image centers 0.0374 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 16:59:51.823 +29:58:47.11
Second-epoch second image center 16:59:53.416 +29:58:28.22
Angular distance between the image centers 0.00778 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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits &> /tmp/tmp.FRchIpLqvQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits &> /tmp/tmp.k17zSGF3sr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits &> /tmp/tmp.HDlIUWRGB5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits &> /tmp/tmp.faNoZR0ewA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
Found non-empty wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
The reference image (wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits) and catalog (wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat) found
'wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat' -> 'wcsmag.cat'
Read 13902 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5508 to 264.5378 deg, Dec +24.5135 to +35.2560 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 245.5508 to 264.5378 deg, Dec 24.5135 to 35.2560 deg
Loaded 9275 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): 6930 out of 7267 total matches.
Matched with Tycho-2 7267 out of 13902 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.819000
a=0.000000 b=1.000000 c=22.819000
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13902 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5508 to 264.5378 deg, Dec +24.5135 to +35.2560 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 245.5508 to 264.5378 deg, Dec 24.5135 to 35.2560 deg
Loaded 9275 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): 6930 out of 7267 total matches.
Matched with Tycho-2 7267 out of 13902 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits:
Forced-photometry filter: calibrated wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits -> calib.txt_param_ref_wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits (aperture=6.2)
Read 12466 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5506 to 264.5030 deg, Dec +24.5138 to +35.2557 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 245.5506 to 264.5030 deg, Dec 24.5138 to 35.2557 deg
Loaded 9255 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): 6896 out of 7217 total matches.
Matched with Tycho-2 7217 out of 12466 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits:
Forced-photometry filter: calibrated wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits -> calib.txt_param_ref_wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits (aperture=6.2)
____ 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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
2.2 pix Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
2.2 pix fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
2.2 pix fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
2.2 pix wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
2.2 pix wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Limiting magnitude estimates:
15.5 mag. Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
15.4 mag. Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
12.4 mag. fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
12.4 mag. fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.0 (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.FRchIpLqvQ (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits' -> 'wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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=844, bad_region=2572, passed=13902
Got 13902 stars (including 10589 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
util/solve_plate_with_UCAC5 got 13902 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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 11518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 11518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 11518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits N_match=973 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.464 n_q1=334 n_q2=149 n_q3=321 n_q4=169 worst_quadrant_to_overall_ratio=1.318
The image catalog is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits -region wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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.k17zSGF3sr (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits' -> 'wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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=801, bad_region=2541, passed=12466
Got 12466 stars (including 9210 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 12466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10144 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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits N_match=974 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.439 sigma_q4_arcsec=0.432 n_q1=332 n_q2=154 n_q3=316 n_q4=172 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits -region wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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.HDlIUWRGB5 (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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=29, bad_region=64, passed=1027
Got 1027 stars (including 934 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 1027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 574 to 628 (Dec 24.8 to 35.2)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 574 to 628 (Dec 24.8 to 35.2)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits N_match=897 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.449 sigma_q3_arcsec=0.604 sigma_q4_arcsec=0.495 n_q1=377 n_q2=253 n_q3=189 n_q4=78 worst_quadrant_to_overall_ratio=1.227
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits -region wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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.faNoZR0ewA (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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=34, bad_region=71, passed=1059
Got 1059 stars (including 957 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 1059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 574 to 628 (Dec 24.8 to 35.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 574 to 628 (Dec 24.8 to 35.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits N_match=929 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.723 sigma_q4_arcsec=0.432 n_q1=401 n_q2=275 n_q3=187 n_q4=66 worst_quadrant_to_overall_ratio=1.518
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits -region wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits sigma_overall=0.352 worst_q_ratio=1.318
ref2=Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits sigma_overall=0.413 worst_q_ratio=1.063
new1=fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits sigma_overall=0.492 worst_q_ratio=1.227
new2=fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits sigma_overall=0.476 worst_q_ratio=1.518
reference average sigma_overall=0.3825 worst_q_ratio=1.1905
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355_astrometric_residuals.png (973 matched stars from wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239_astrometric_residuals.png (974 matched stars from wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248_astrometric_residuals.png (897 matched stars from wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249_astrometric_residuals.png (929 matched stars from wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits'
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits'
Preparing the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Her-04-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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Creating symlink local_wcs_cache/wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Creating symlink local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Creating symlink local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits exists and is non-empty
wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits exists and is non-empty
wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits exists and is non-empty
wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits (1st reference image)
verification OK: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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: 17:00:01.882 +29:59:45.68 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-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Image size: 937.5'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: 16:59:51.823 +29:58:47.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:00:01.882 +29:59:45.68
Second-epoch image center 16:59:51.823 +29:58:47.11
Angular distance between the image centers 0.0398 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Image size: 937.5'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: 16:59:53.416 +29:58:28.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:00:01.882 +29:59:45.68
Second-epoch image center 16:59:53.416 +29:58:28.22
Angular distance between the image centers 0.0374 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 16:59:51.823 +29:58:47.11
Second-epoch second image center 16:59:53.416 +29:58:28.22
Angular distance between the image centers 0.00778 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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits &> /tmp/tmp.sz4EjBD1PO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits &> /tmp/tmp.kpCyAEbox0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits &> /tmp/tmp.NCbCUM5kuA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits &> /tmp/tmp.ku8PHxYiEH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
Found non-empty wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits and wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
The reference image (wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits) and catalog (wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat) found
'wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat' -> 'wcsmag.cat'
Read 76127 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5378 to 264.5378 deg, Dec +24.4901 to +35.2605 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 245.5378 to 264.5378 deg, Dec 24.4901 to 35.2605 deg
Loaded 9308 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): 6377 out of 7307 total matches.
Matched with Tycho-2 7307 out of 76127 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.694000
a=0.000000 b=1.000000 c=22.694000
From vast_summary.log: estimated ref. image limiting mag.: -7.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 76127 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5378 to 264.5378 deg, Dec +24.4901 to +35.2605 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 245.5378 to 264.5378 deg, Dec 24.4901 to 35.2605 deg
Loaded 9308 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): 6377 out of 7307 total matches.
Matched with Tycho-2 7307 out of 76127 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits:
Forced-photometry filter: calibrated wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits -> calib.txt_param_ref_wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits (aperture=4.8)
Read 75369 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.5385 to 264.5376 deg, Dec +24.4912 to +35.2609 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 245.5385 to 264.5376 deg, Dec 24.4912 to 35.2609 deg
Loaded 9307 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): 6377 out of 7304 total matches.
Matched with Tycho-2 7304 out of 75369 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits:
Forced-photometry filter: calibrated wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits -> calib.txt_param_ref_wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 177 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
2.1 pix Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
2.1 pix fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
2.0 pix fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
2.2 pix wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
2.1 pix wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Limiting magnitude estimates:
15.6 mag. Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
15.5 mag. Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
12.7 mag. fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
13.0 mag. fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sz4EjBD1PO (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits' -> 'wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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=10, blended=4941, bad_region=10350, passed=76117
Got 76117 stars (including 61522 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat
util/solve_plate_with_UCAC5 got 76117 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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 66778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 66778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 66777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits N_match=975 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.468 n_q1=328 n_q2=155 n_q3=327 n_q4=165 worst_quadrant_to_overall_ratio=1.292
The image catalog is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits -region wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.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.kpCyAEbox0 (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits' -> 'wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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=33, blended=4620, bad_region=10713, passed=75336
Got 75336 stars (including 60580 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 75336 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 65780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 65780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 65780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits N_match=974 sigma_overall_arcsec=0.445 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.465 sigma_q4_arcsec=0.484 n_q1=319 n_q2=160 n_q3=327 n_q4=168 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits -region wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.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.NCbCUM5kuA (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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=151, bad_region=467, passed=9350
Got 9350 stars (including 8749 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 9350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 572 to 628 (Dec 24.5 to 35.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 8641 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 572 to 628 (Dec 24.5 to 35.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits N_match=960 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.467 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.599 sigma_q4_arcsec=0.494 n_q1=416 n_q2=246 n_q3=216 n_q4=82 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits -region wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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.ku8PHxYiEH (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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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=2, blended=191, bad_region=491, passed=9847
Got 9847 stars (including 9180 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 9847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 572 to 628 (Dec 24.5 to 35.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 9141 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 572 to 628 (Dec 24.5 to 35.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits N_match=964 sigma_overall_arcsec=0.452 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.390 sigma_q3_arcsec=0.650 sigma_q4_arcsec=0.424 n_q1=443 n_q2=250 n_q3=207 n_q4=64 worst_quadrant_to_overall_ratio=1.439
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits -region wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/wcs_fd_Her-04-Q2b1x1_2026-07-16_03-59-21_20.00sec_4.90C_LIGHT_0248.fits
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.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-04-Q2b1x1_040032_TTUQ2b1x1_29537_6ZZFHiws/wcs_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249.fits
Preparing the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:14.18 +33:14:12.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:24.98 +29:35:16.5: 13.39 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:28.50 +33:25:21.0: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:01.08 +32:54:16.1: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:49.35 +33:23:53.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:16.52 +33:28:27.0: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:22.77 +33:21:21.4: 13.78 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:39.43 +33:08:00.9: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:00.01 +33:39:18.1: 14.19 +/- 0.06 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:16.16 +33:31:06.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:24.98 +29:35:16.5: 13.38 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:28.50 +33:25:21.0: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 17:09:24.98 +29:35:16.5: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3867 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:28.50 +33:25:21.0: ref_mag=13.57 +/- 0.02 new_mean_mag=12.4711 delta=1.10 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:14.18 +33:14:12.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:01.08 +32:54:16.1: 13.77 +/- 0.04 detection
Forced photometry filter KEPT candidate at 17:11:14.18 +33:14:12.5: ref_mag=13.28 +/- 0.02 new_mean_mag=12.0858 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:49.35 +33:23:53.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 17:12:01.08 +32:54:16.1: ref_mag=13.76 +/- 0.03 new_mean_mag=12.6198 delta=1.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 17:10:49.35 +33:23:53.6: ref_mag=13.06 +/- 0.01 new_mean_mag=12.0245 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:39.43 +33:08:00.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:00.01 +33:39:18.1: 14.16 +/- 0.06 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:16.52 +33:28:27.0: 13.26 +/- 0.02 detection
Forced photometry filter KEPT candidate at 17:12:39.43 +33:08:00.9: ref_mag=13.02 +/- 0.01 new_mean_mag=12.0790 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:22.77 +33:21:21.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:16.52 +33:28:27.0: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3491 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 17:11:00.01 +33:39:18.1: ref_mag=14.17 +/- 0.04 new_mean_mag=12.7479 delta=1.43 (need > 0.90)
Forced photometry filter KEPT candidate at 17:11:22.77 +33:21:21.4: ref_mag=13.85 +/- 0.03 new_mean_mag=12.6071 delta=1.24 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:16.16 +33:31:06.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:16.16 +33:31:06.0: ref_mag=13.06 +/- 0.01 new_mean_mag=12.0990 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:45.53 +32:56:29.7: 14.03 +/- 0.05 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:18.37 +33:14:52.7: 12.57 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:25.97 +29:39:38.7: 13.45 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:45.53 +32:56:29.7: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.03
Forced photometry filter KEPT candidate at 17:11:45.53 +32:56:29.7: ref_mag=14.03 +/- 0.03 new_mean_mag=12.5317 delta=1.50 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:18.37 +33:14:52.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 17:07:18.37 +33:14:52.7: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5709 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:25.97 +29:39:38.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:25.97 +29:39:38.7: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4259 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:28.03 +33:05:40.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:28.03 +33:05:40.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 17:12:28.03 +33:05:40.4: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9458 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:19.66 +33:00:20.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:19.66 +33:00:20.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 17:12:19.66 +33:00:20.6: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9679 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:47.49 +30:47:13.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:09.09 +33:26:06.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:24.43 +33:25:56.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:25.55 +33:24:33.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:47.49 +30:47:13.1: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:47.49 +30:47:13.1: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9250 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:09.09 +33:26:06.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:09.09 +33:26:06.4: ref_mag=12.94 +/- 0.01 new_mean_mag=11.9896 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:24.43 +33:25:56.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:24.43 +33:25:56.7: ref_mag=12.92 +/- 0.01 new_mean_mag=11.9543 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:22.78 +30:05:37.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:27.62 +33:15:55.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:25.55 +33:24:33.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 17:07:25.55 +33:24:33.5: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8973 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:22.78 +30:05:37.2: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:22.78 +30:05:37.2: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8738 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:27.62 +33:15:55.4: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.02
Forced photometry filter KEPT candidate at 17:10:27.62 +33:15:55.4: ref_mag=13.67 +/- 0.02 new_mean_mag=12.5425 delta=1.13 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:32.34 +30:01:35.5: 13.26 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:18.29 +30:59:26.7: 13.25 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:18.29 +30:59:26.7: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:32.34 +30:01:35.5: 13.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 17:09:18.29 +30:59:26.7: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3309 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 17:08:32.34 +30:01:35.5: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2639 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:32.44 +30:41:57.9: 12.88 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:32.44 +30:41:57.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:32.44 +30:41:57.9: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9175 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:09.66 +33:31:32.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:36.63 +33:25:16.0: 12.86 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:09.66 +33:31:32.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 17:04:09.66 +33:31:32.2: ref_mag=12.86 +/- 0.01 new_mean_mag=11.9120 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:36.63 +33:25:16.0: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:36.63 +33:25:16.0: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8784 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:02:09.67 +33:21:45.3: 13.24 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:02:09.67 +33:21:45.3: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 17:02:09.67 +33:21:45.3: ref_mag=13.24 +/- 0.02 new_mean_mag=12.3102 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:57.38 +32:51:28.7: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:24.22 +29:44:49.6: 13.53 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:57.38 +32:51:28.7: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:57.38 +32:51:28.7: ref_mag=13.49 +/- 0.02 new_mean_mag=12.3193 delta=1.17 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:24.22 +29:44:49.6: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:24.22 +29:44:49.6: ref_mag=13.53 +/- 0.02 new_mean_mag=12.2509 delta=1.28 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:15.76 +31:06:12.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:15.76 +31:06:12.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:10:15.76 +31:06:12.2: ref_mag=13.50 +/- 0.02 new_mean_mag=12.4428 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:05.78 +29:00:57.3: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:05.78 +29:00:57.3: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:09:05.78 +29:00:57.3: ref_mag=13.50 +/- 0.02 new_mean_mag=12.2907 delta=1.21 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:06.76 +33:23:58.8: 13.49 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:06.76 +33:23:58.8: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 17:05:06.76 +33:23:58.8: ref_mag=13.49 +/- 0.02 new_mean_mag=12.4835 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:53.26 +34:10:33.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:53.26 +34:10:33.7: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 17:05:53.26 +34:10:33.7: ref_mag=13.51 +/- 0.02 new_mean_mag=12.4517 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:45.60 +33:03:03.3: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:45.60 +33:03:03.3: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 17:04:45.60 +33:03:03.3: ref_mag=12.84 +/- 0.01 new_mean_mag=11.9249 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:12.06 +34:05:25.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:12.06 +34:05:25.8: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 16:47:12.06 +34:05:25.8: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2289 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:54.25 +33:00:21.5: 12.84 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:54.25 +33:00:21.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 17:11:54.25 +33:00:21.5: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8385 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:03.11 +32:50:52.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:03.11 +32:50:52.9: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:03.11 +32:50:52.9: ref_mag=13.66 +/- 0.02 new_mean_mag=12.6364 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:11.85 +33:01:53.6: 13.45 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:11.85 +33:01:53.6: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 17:12:11.85 +33:01:53.6: ref_mag=13.45 +/- 0.02 new_mean_mag=12.3049 delta=1.15 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:07.25 +29:48:40.8: 13.23 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:00.37 +30:12:15.5: 13.22 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:07.25 +29:48:40.8: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 17:09:07.25 +29:48:40.8: ref_mag=13.21 +/- 0.02 new_mean_mag=12.0992 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:00.37 +30:12:15.5: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:00.37 +30:12:15.5: ref_mag=13.23 +/- 0.02 new_mean_mag=12.1494 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:50.75 +30:50:48.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:34.31 +33:14:07.2: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:50.75 +30:50:48.7: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:50.75 +30:50:48.7: ref_mag=13.42 +/- 0.02 new_mean_mag=12.2067 delta=1.21 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:34.31 +33:14:07.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:34.31 +33:14:07.2: ref_mag=13.18 +/- 0.01 new_mean_mag=12.0245 delta=1.16 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:11.23 +33:17:09.1: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:03:59.55 +33:40:18.9: 13.67 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:11.23 +33:17:09.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 17:10:11.23 +33:17:09.1: ref_mag=13.24 +/- 0.02 new_mean_mag=12.3161 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:03:59.55 +33:40:18.9: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 17:03:59.55 +33:40:18.9: ref_mag=13.66 +/- 0.02 new_mean_mag=12.5472 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:24.30 +33:30:35.2: 13.18 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:51.71 +33:48:07.4: 13.22 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:24.30 +33:30:35.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:24.30 +33:30:35.2: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2513 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:16.92 +32:19:47.4: 12.55 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:51.71 +33:48:07.4: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:51.71 +33:48:07.4: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2626 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:16.92 +32:19:47.4: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:16.92 +32:19:47.4: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5665 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:31.05 +28:44:41.8: 13.88 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:31.05 +28:44:41.8: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 17:08:31.05 +28:44:41.8: ref_mag=13.85 +/- 0.03 new_mean_mag=12.5525 delta=1.30 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:13.17 +33:24:33.7: 13.18 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:13.17 +33:24:33.7: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 17:10:13.17 +33:24:33.7: ref_mag=13.19 +/- 0.02 new_mean_mag=12.0701 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:15.57 +33:08:46.1: 12.80 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:15.57 +33:08:46.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 17:11:15.57 +33:08:46.1: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7276 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:56.84 +32:23:44.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:56.84 +32:23:44.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:56.84 +32:23:44.8: ref_mag=13.41 +/- 0.02 new_mean_mag=12.2649 delta=1.15 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:10:57.22 +32:41:11.6: 13.41 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:10:57.22 +32:41:11.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 17:10:57.22 +32:41:11.6: ref_mag=13.38 +/- 0.02 new_mean_mag=12.4093 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:03.59 +33:07:34.4: 12.80 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:46.70 +33:03:22.5: 13.86 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:03.59 +33:07:34.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 17:07:03.59 +33:07:34.4: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7330 delta=1.07 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:46.70 +33:03:22.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 17:11:46.70 +33:03:22.5: ref_mag=13.89 +/- 0.03 new_mean_mag=12.5460 delta=1.35 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:17.62 +33:24:58.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:17.62 +33:24:58.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 17:05:17.62 +33:24:58.8: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5382 delta=1.13 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:44.99 +33:00:31.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:44.99 +33:00:31.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:44.99 +33:00:31.9: ref_mag=13.17 +/- 0.01 new_mean_mag=12.0411 delta=1.13 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:04.36 +34:08:54.9: 13.15 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:04.36 +34:08:54.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 16:47:04.36 +34:08:54.9: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1035 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:25.39 +30:41:12.9: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:25.39 +30:41:12.9: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:25.39 +30:41:12.9: ref_mag=13.15 +/- 0.01 new_mean_mag=12.1037 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:43.70 +33:16:07.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:43.70 +33:16:07.8: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:43.70 +33:16:07.8: ref_mag=13.16 +/- 0.02 new_mean_mag=12.0768 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:01.01 +33:32:19.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:01.01 +33:32:19.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:01.01 +33:32:19.0: ref_mag=13.08 +/- 0.01 new_mean_mag=12.1150 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:58.22 +33:29:38.1: 13.65 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:58.22 +33:29:38.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:58.22 +33:29:38.1: ref_mag=13.65 +/- 0.02 new_mean_mag=12.5472 delta=1.10 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:06.93 +33:13:21.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:34.43 +29:51:55.1: 13.41 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:06.93 +33:13:21.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 17:12:06.93 +33:13:21.4: ref_mag=13.11 +/- 0.01 new_mean_mag=12.0174 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:34.43 +29:51:55.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:34.43 +29:51:55.1: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3369 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:32.02 +33:18:42.1: 12.46 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:59.49 +33:48:36.2: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:32.02 +33:18:42.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:32.02 +33:18:42.1: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4500 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:59.49 +33:48:36.2: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 17:05:59.49 +33:48:36.2: ref_mag=13.66 +/- 0.02 new_mean_mag=12.5228 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:18.90 +30:41:27.7: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:18.90 +30:41:27.7: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:18.90 +30:41:27.7: ref_mag=13.10 +/- 0.01 new_mean_mag=12.1016 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:49:11.27 +34:05:49.8: 13.81 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:49:11.27 +34:05:49.8: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter KEPT candidate at 16:49:11.27 +34:05:49.8: ref_mag=13.87 +/- 0.03 new_mean_mag=12.6892 delta=1.18 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:11.02 +29:58:39.1: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:11.02 +29:58:39.1: 13.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter KEPT candidate at 17:07:11.02 +29:58:39.1: ref_mag=13.65 +/- 0.02 new_mean_mag=12.4458 delta=1.21 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:24.82 +30:44:45.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:24.82 +30:44:45.5: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:24.82 +30:44:45.5: ref_mag=13.04 +/- 0.01 new_mean_mag=12.0299 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:54.56 +33:01:16.8: 13.08 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:54.56 +33:01:16.8: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 17:04:54.56 +33:01:16.8: ref_mag=13.06 +/- 0.01 new_mean_mag=12.1163 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:40.59 +32:53:35.0: 12.42 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:40.59 +32:53:35.0: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:58.11 +30:45:51.3: 13.39 +/- 0.02 detection
Forced photometry filter KEPT candidate at 17:11:40.59 +32:53:35.0: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4180 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:30.39 +30:46:17.1: 13.11 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:58.11 +30:45:51.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:58.11 +30:45:51.3: ref_mag=13.41 +/- 0.02 new_mean_mag=12.2649 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:30.39 +30:46:17.1: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:30.39 +30:46:17.1: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1021 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:46:29.13 +34:11:02.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:46:29.13 +34:11:02.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 16:46:29.13 +34:11:02.0: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3673 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:55.29 +33:04:25.0: 12.39 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:55.29 +33:04:25.0: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:55.29 +33:04:25.0: ref_mag=12.37 +/- 0.01 new_mean_mag=11.3927 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:30.81 +33:17:46.4: 11.72 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:30.81 +33:17:46.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Forced photometry filter KEPT candidate at 17:06:30.81 +33:17:46.4: ref_mag=11.72 +/- 0.00 new_mean_mag=10.8068 delta=0.91 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:10.85 +33:19:39.7: 12.36 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:10.85 +33:19:39.7: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 17:07:10.85 +33:19:39.7: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3560 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:27.77 +29:13:06.2: 12.35 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:43.56 +33:05:11.4: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:27.77 +29:13:06.2: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:27.77 +29:13:06.2: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4014 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:43.56 +33:05:11.4: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 17:11:43.56 +33:05:11.4: ref_mag=12.33 +/- 0.01 new_mean_mag=11.3939 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:25.83 +33:15:13.4: 13.36 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:46.11 +33:54:06.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:25.83 +33:15:13.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:25.83 +33:15:13.4: ref_mag=13.38 +/- 0.02 new_mean_mag=12.2425 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:46.11 +33:54:06.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:46.11 +33:54:06.9: ref_mag=13.36 +/- 0.02 new_mean_mag=12.4285 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:33.52 +30:04:40.2: 13.36 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:57.60 +33:19:49.2: 13.82 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:33.52 +30:04:40.2: 13.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 17:07:33.52 +30:04:40.2: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3511 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:44.43 +30:04:19.6: 13.79 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:57.60 +33:19:49.2: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 17:04:57.60 +33:19:49.2: ref_mag=13.78 +/- 0.03 new_mean_mag=12.5463 delta=1.23 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:44.43 +30:04:19.6: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 17:07:44.43 +30:04:19.6: ref_mag=13.80 +/- 0.03 new_mean_mag=12.5696 delta=1.23 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:41.79 +33:17:50.4: 13.35 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:41.79 +33:17:50.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 17:09:41.79 +33:17:50.4: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3620 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:13.94 +33:03:51.5: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:13.94 +33:03:51.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 17:12:13.94 +33:03:51.5: ref_mag=13.33 +/- 0.02 new_mean_mag=12.2430 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:08.08 +33:06:06.5: 12.74 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:08.08 +33:06:06.5: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 17:12:08.08 +33:06:06.5: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7029 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:00.51 +28:58:38.0: 12.30 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:00.51 +28:58:38.0: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:00.51 +28:58:38.0: ref_mag=12.32 +/- 0.01 new_mean_mag=11.2525 delta=1.07 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:18.97 +33:36:25.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:18.97 +33:36:25.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:04:18.97 +33:36:25.8: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2661 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:01.17 +33:37:55.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:01.17 +33:37:55.5: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:01.17 +33:37:55.5: ref_mag=13.07 +/- 0.01 new_mean_mag=12.1192 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:14.08 +33:57:01.5: 13.33 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:14.08 +33:57:01.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 16:47:14.08 +33:57:01.5: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3337 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:12:51.96 +33:08:50.5: 12.71 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:12:51.96 +33:08:50.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 17:12:51.96 +33:08:50.5: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7669 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:06.02 +32:55:02.9: 12.72 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:44.12 +29:26:08.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:44.12 +29:26:08.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:06.02 +32:55:02.9: 12.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:44.12 +29:26:08.0: ref_mag=13.06 +/- 0.01 new_mean_mag=12.0987 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 17:11:06.02 +32:55:02.9: ref_mag=12.71 +/- 0.01 new_mean_mag=11.6512 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:45:39.59 +33:23:43.6: 13.33 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:45:39.59 +33:23:43.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 16:45:39.59 +33:23:43.6: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3049 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:35.66 +29:01:03.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:35.66 +29:01:03.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:35.66 +29:01:03.1: ref_mag=12.71 +/- 0.01 new_mean_mag=11.6884 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:07:06.02 +33:17:01.5: 12.26 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:07:06.02 +33:17:01.5: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 17:07:06.02 +33:17:01.5: ref_mag=12.26 +/- 0.01 new_mean_mag=11.3205 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:54.15 +33:12:37.1: 13.32 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:42.56 +33:07:19.6: 11.53 +/- 0.00 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:54.15 +33:12:37.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 17:06:54.15 +33:12:37.1: ref_mag=13.34 +/- 0.02 new_mean_mag=12.1501 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:42.56 +33:07:19.6: 11.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Forced photometry filter KEPT candidate at 17:06:42.56 +33:07:19.6: ref_mag=11.53 +/- 0.00 new_mean_mag=10.6003 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:28.51 +33:09:44.5: 13.54 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:58.12 +30:01:17.6: 13.78 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:28.51 +33:09:44.5: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:28.51 +33:09:44.5: ref_mag=13.50 +/- 0.02 new_mean_mag=12.2765 delta=1.23 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:58.12 +30:01:17.6: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 17:06:58.12 +30:01:17.6: ref_mag=13.78 +/- 0.03 new_mean_mag=12.4507 delta=1.32 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:03.04 +32:57:29.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:03.04 +32:57:29.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:03.04 +32:57:29.9: ref_mag=13.01 +/- 0.01 new_mean_mag=12.0745 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:52.50 +30:01:20.3: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:52.50 +30:01:20.3: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 17:06:52.50 +30:01:20.3: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2199 delta=1.07 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:26.43 +32:52:03.2: 13.29 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:26.43 +32:52:03.2: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:26.43 +32:52:03.2: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3157 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:52.59 +29:00:53.4: 12.67 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:52.59 +29:00:53.4: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:52.59 +29:00:53.4: ref_mag=12.70 +/- 0.01 new_mean_mag=11.5825 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:45.76 +28:57:14.7: 12.21 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:45.76 +28:57:14.7: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:45.76 +28:57:14.7: ref_mag=12.21 +/- 0.01 new_mean_mag=11.1532 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:58.77 +33:18:36.1: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:58.77 +33:18:36.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 17:05:58.77 +33:18:36.1: ref_mag=13.55 +/- 0.02 new_mean_mag=12.3883 delta=1.16 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:56.32 +33:04:28.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:56.32 +33:04:28.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 17:11:56.32 +33:04:28.0: ref_mag=13.74 +/- 0.03 new_mean_mag=12.4919 delta=1.25 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:05:09.06 +33:40:36.0: 12.66 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:52.54 +33:02:08.3: 13.74 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:05:09.06 +33:40:36.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 17:05:09.06 +33:40:36.0: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6906 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:52.54 +33:02:08.3: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 17:06:52.54 +33:02:08.3: ref_mag=13.66 +/- 0.02 new_mean_mag=12.3098 delta=1.35 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:09:11.81 +32:29:34.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:04:06.59 +33:35:50.0: 13.91 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:01.39 +33:20:25.7: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:09:11.81 +32:29:34.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 17:09:11.81 +32:29:34.4: ref_mag=12.98 +/- 0.01 new_mean_mag=11.9008 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:04:06.59 +33:35:50.0: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 17:04:06.59 +33:35:50.0: ref_mag=13.86 +/- 0.03 new_mean_mag=12.5370 delta=1.32 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:01.39 +33:20:25.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:06:01.39 +33:20:25.7: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2515 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:06:17.78 +33:31:35.9: 13.00 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:06:17.78 +33:31:35.9: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 17:06:17.78 +33:31:35.9: ref_mag=12.96 +/- 0.01 new_mean_mag=12.0167 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:04.90 +29:28:13.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:04.90 +29:28:13.4: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 17:08:04.90 +29:28:13.4: ref_mag=13.75 +/- 0.03 new_mean_mag=12.4484 delta=1.31 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:51.14 +28:50:33.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:51.14 +28:50:33.5: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 17:08:51.14 +28:50:33.5: ref_mag=13.72 +/- 0.03 new_mean_mag=12.5211 delta=1.20 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 16:47:24.01 +34:06:33.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 16:47:24.01 +34:06:33.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 16:47:24.01 +34:06:33.3: ref_mag=12.96 +/- 0.01 new_mean_mag=11.9505 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:02:20.65 +33:06:43.1: 13.28 +/- 0.02 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:02:20.65 +33:06:43.1: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 17:02:20.65 +33:06:43.1: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3229 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:18.92 +33:09:56.5: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:18.92 +33:09:56.5: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:18.92 +33:09:56.5: ref_mag=13.48 +/- 0.02 new_mean_mag=12.2330 delta=1.25 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:49.14 +28:53:39.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:49.14 +28:53:39.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 17:08:49.14 +28:53:39.8: ref_mag=12.61 +/- 0.01 new_mean_mag=11.4770 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:11:33.99 +33:36:56.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-05-12_03-45-42_20.00sec_-5.00C_LIGHT_0355.fits at 17:08:43.44 +30:13:57.1: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:11:33.99 +33:36:56.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:11:33.99 +33:36:56.4: ref_mag=13.50 +/- 0.02 new_mean_mag=12.3823 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-04-Q2b1x1_2026-06-21_01-46-05_20.00sec_4.90C_LIGHT_0239.fits at 17:08:43.44 +30:13:57.1: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 17:08:43.44 +30:13:57.1: ref_mag=13.54 +/- 0.02 new_mean_mag=12.3904 delta=1.14 (need > 0.90)
Adding exclusion_list_local.txt__out06475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56070.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 230s
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: 60s
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Considering the candidate 91008_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91008_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
**** FOUND 17:00:23.88 +30:56:43.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 91014_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91014_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 91016_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91016_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 91019_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91019_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 91032_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91032_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 91033_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91033_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 91035_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91035_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 91039_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91039_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (35.2") between the two second-epoch detections
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Considering the candidate 91042_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91042_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 91049_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91049_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 91051_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91051_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 91054_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91054_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 91055_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91055_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 91060_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91060_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 91068_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91068_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 91070_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91070_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 91071_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91071_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 91075_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91075_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 91077_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91077_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 91078_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91078_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 91081_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91081_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 91084_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91084_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 91089_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91089_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
**** FOUND 16:43:45.80 +34:02:39.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91091_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91091_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 91092_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91092_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
**** FOUND 16:53:03.17 +31:42:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91095_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91095_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 91098_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91098_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 91103_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91103_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 91104_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91104_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 91105_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91105_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 91108_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91108_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 91111_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91111_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 91114_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91114_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 91115_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91115_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
**** FOUND 16:46:16.16 +33:48:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91117_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91117_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 91121_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91121_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 91122_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91122_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 91126_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91126_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 91127_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91127_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 91128_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91128_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 91129_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91129_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 91135_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91135_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 91137_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91137_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 91138_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91138_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 91147_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91147_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 91151_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91151_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (47.5") between the two second-epoch detections
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Considering the candidate 91152_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91152_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 91154_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91154_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 91155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 91157_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91157_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
**** FOUND 16:50:32.25 +29:46:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91161_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91161_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 91166_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91166_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 91172_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 91172_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 11889_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11889_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12887_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12887_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11567_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11567_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12155_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11849_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11849_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13527_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13527_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10085_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10085_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 40015_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 40015_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11159_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11159_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14908_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14908_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12964_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12964_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 39473_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 39473_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13762_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13762_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14372_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14372_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 30923_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 30923_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11800_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11800_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 69527_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 69527_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 11769_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11769_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11911_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11911_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12794_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12794_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36136_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36136_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36673_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36673_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 29317_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 29317_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31628_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31628_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11134_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11134_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11868_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11868_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12346_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12346_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15457_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15457_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 38865_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 38865_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 28457_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 28457_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 44440_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 44440_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12045_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12045_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 06678_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 06678_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14285_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14285_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 07076_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 07076_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14360_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14360_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15585_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15585_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14196_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14196_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 38327_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 38327_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 35413_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 35413_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 30441_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 30441_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13121_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13121_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12633_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12633_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10178_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10178_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11064_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11064_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 09201_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 09201_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 19404_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 19404_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 54968_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 54968_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11801_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11801_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13506_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13506_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 18958_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 18958_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 16769_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 16769_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13716_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13716_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14069_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14069_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11924_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11924_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14581_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14581_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 06686_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 06686_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31729_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31729_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12701_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12701_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11048_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11048_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11407_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11407_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12974_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12974_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 37935_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 37935_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12529_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12529_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 09154_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 09154_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31703_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31703_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 07150_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 07150_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 37067_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 37067_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31228_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31228_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14507_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14507_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15192_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15192_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31109_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31109_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 31067_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 31067_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 06475_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 06475_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 23959_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
The candidate 23959_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 14045_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14045_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12570_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12570_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12389_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12389_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 42789_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 42789_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13853_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13853_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12806_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12806_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 08517_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 08517_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36307_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36307_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12489_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12489_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36391_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36391_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12602_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12602_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13981_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13981_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13724_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13724_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 44670_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 44670_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10628_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10628_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10392_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10392_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 08080_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 08080_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13389_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13389_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15035_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15035_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 41165_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 41165_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11824_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11824_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 44338_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 44338_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12712_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12712_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13236_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13236_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13740_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13740_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13414_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13414_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36766_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36766_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14989_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14989_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 36716_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 36716_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 15453_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 15453_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 44385_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 44385_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 44832_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 44832_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12610_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12610_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13952_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13952_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10098_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10098_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 14371_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 14371_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 18185_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 18185_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10689_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10689_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 12408_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 12408_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 11077_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 11077_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 40962_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 40962_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 55675_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 55675_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 06968_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 06968_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13773_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13773_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 13373_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 13373_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 56070_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 56070_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 10316_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 10316_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
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Considering the candidate 35164_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
Preparing report for the candidate 35164_fd_Her-04-Q2b1x1_2026-07-16_04-00-03_20.00sec_4.90C_LIGHT_0249
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 300s
Prepared the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:46:29.13 +34:11:02.0
17:05:53.26 +34:10:33.7
16:47:04.36 +34:08:54.9
16:47:24.01 +34:06:33.3
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16:47:14.08 +33:57:01.5
17:04:46.11 +33:54:06.9
17:05:59.49 +33:48:36.2
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17:03:59.55 +33:40:18.9
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17:05:01.17 +33:37:55.5
17:04:18.97 +33:36:25.8
17:04:06.59 +33:35:50.0
17:05:01.01 +33:32:19.0
17:11:24.30 +33:30:35.2
17:06:17.78 +33:31:35.9
17:04:09.66 +33:31:32.2
17:06:16.16 +33:31:06.0
17:04:58.22 +33:29:38.1
17:04:16.52 +33:28:27.0
17:05:09.09 +33:26:06.4
17:05:24.43 +33:25:56.7
17:10:13.17 +33:24:33.7
16:45:39.59 +33:23:43.6
17:10:49.35 +33:23:53.6
17:05:36.63 +33:25:16.0
17:04:28.50 +33:25:21.0
17:07:25.55 +33:24:33.5
17:05:17.62 +33:24:58.8
17:05:06.76 +33:23:58.8
17:11:22.77 +33:21:21.4
17:02:09.67 +33:21:45.3
17:07:10.85 +33:19:39.7
17:06:01.39 +33:20:25.7
17:04:57.60 +33:19:49.2
17:06:32.02 +33:18:42.1
17:06:30.81 +33:17:46.4
17:09:41.79 +33:17:50.4
17:05:58.77 +33:18:36.1
17:10:11.23 +33:17:09.1
17:11:43.70 +33:16:07.8
17:07:06.02 +33:17:01.5
17:10:27.62 +33:15:55.4
17:11:25.83 +33:15:13.4
17:11:14.18 +33:14:12.5
17:07:18.37 +33:14:52.7
17:12:06.93 +33:13:21.4
17:05:34.31 +33:14:07.2
17:06:54.15 +33:12:37.1
17:11:18.92 +33:09:56.5
17:12:51.96 +33:08:50.5
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17:12:39.43 +33:08:00.9
17:07:03.59 +33:07:34.4
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17:06:42.56 +33:07:19.6
17:12:28.03 +33:05:40.4
17:02:20.65 +33:06:43.1
17:11:43.56 +33:05:11.4
17:11:56.32 +33:04:28.0
17:12:13.94 +33:03:51.5
17:06:55.29 +33:04:25.0
17:11:46.70 +33:03:22.5
17:12:11.85 +33:01:53.6
17:04:45.60 +33:03:03.3
17:11:54.25 +33:00:21.5
17:06:52.54 +33:02:08.3
17:12:19.66 +33:00:20.6
17:04:54.56 +33:01:16.8
17:05:44.99 +33:00:31.9
17:11:45.53 +32:56:29.7
17:05:03.04 +32:57:29.9
17:11:06.02 +32:55:02.9
17:12:01.08 +32:54:16.1
17:11:40.59 +32:53:35.0
17:08:26.43 +32:52:03.2
17:11:57.38 +32:51:28.7
17:11:03.11 +32:50:52.9
17:10:57.22 +32:41:11.6
17:09:11.81 +32:29:34.4
17:08:56.84 +32:23:44.8
17:09:16.92 +32:19:47.4
17:10:15.76 +31:06:12.2
17:09:18.29 +30:59:26.7
17:08:50.75 +30:50:48.7
17:08:47.49 +30:47:13.1
17:08:30.39 +30:46:17.1
17:08:58.11 +30:45:51.3
17:09:24.82 +30:44:45.5
17:08:32.44 +30:41:57.9
17:08:18.90 +30:41:27.7
17:08:25.39 +30:41:12.9
17:08:43.44 +30:13:57.1
17:08:00.37 +30:12:15.5
17:08:22.78 +30:05:37.2
17:07:33.52 +30:04:40.2
17:07:44.43 +30:04:19.6
17:08:32.34 +30:01:35.5
17:06:52.50 +30:01:20.3
17:06:58.12 +30:01:17.6
17:07:11.02 +29:58:39.1
17:08:34.43 +29:51:55.1
17:09:07.25 +29:48:40.8
17:08:24.22 +29:44:49.6
17:08:25.97 +29:39:38.7
17:09:24.98 +29:35:16.5
17:08:04.90 +29:28:13.4
17:09:44.12 +29:26:08.0
17:09:27.77 +29:13:06.2
17:09:35.66 +29:01:03.1
17:08:52.59 +29:00:53.4
17:09:05.78 +29:00:57.3
17:09:00.51 +28:58:38.0
17:08:45.76 +28:57:14.7
17:08:31.05 +28:44:41.8
17:08:51.14 +28:50:33.5
17:08:49.14 +28:53:39.8
########### Completed Her-04-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 ####
17:04:28.50 +33:25:21.0
17:12:01.08 +32:54:16.1
17:11:14.18 +33:14:12.5
17:04:16.52 +33:28:27.0
17:11:22.77 +33:21:21.4
17:10:49.35 +33:23:53.6
17:12:39.43 +33:08:00.9
17:11:00.01 +33:39:18.1
17:09:24.98 +29:35:16.5
17:06:16.16 +33:31:06.0
17:11:45.53 +32:56:29.7
17:07:18.37 +33:14:52.7
17:08:25.97 +29:39:38.7
17:12:28.03 +33:05:40.4
17:12:19.66 +33:00:20.6
17:08:47.49 +30:47:13.1
17:05:24.43 +33:25:56.7
17:05:09.09 +33:26:06.4
17:07:25.55 +33:24:33.5
17:10:27.62 +33:15:55.4
17:08:22.78 +30:05:37.2
17:08:32.34 +30:01:35.5
17:09:18.29 +30:59:26.7
17:08:32.44 +30:41:57.9
17:04:09.66 +33:31:32.2
17:05:36.63 +33:25:16.0
17:02:09.67 +33:21:45.3
17:11:57.38 +32:51:28.7
17:08:24.22 +29:44:49.6
17:10:15.76 +31:06:12.2
17:09:05.78 +29:00:57.3
17:05:06.76 +33:23:58.8
17:05:53.26 +34:10:33.7
17:04:45.60 +33:03:03.3
16:47:12.06 +34:05:25.8
17:11:54.25 +33:00:21.5
17:11:03.11 +32:50:52.9
17:12:11.85 +33:01:53.6
17:09:07.25 +29:48:40.8
17:08:00.37 +30:12:15.5
17:08:50.75 +30:50:48.7
17:05:34.31 +33:14:07.2
17:10:11.23 +33:17:09.1
17:03:59.55 +33:40:18.9
17:11:24.30 +33:30:35.2
17:04:51.71 +33:48:07.4
17:09:16.92 +32:19:47.4
17:08:31.05 +28:44:41.8
17:10:13.17 +33:24:33.7
17:11:15.57 +33:08:46.1
17:08:56.84 +32:23:44.8
17:10:57.22 +32:41:11.6
17:07:03.59 +33:07:34.4
17:11:46.70 +33:03:22.5
17:05:17.62 +33:24:58.8
17:05:44.99 +33:00:31.9
16:47:04.36 +34:08:54.9
17:08:25.39 +30:41:12.9
17:11:43.70 +33:16:07.8
17:05:01.01 +33:32:19.0
17:04:58.22 +33:29:38.1
17:12:06.93 +33:13:21.4
17:08:34.43 +29:51:55.1
17:06:32.02 +33:18:42.1
17:05:59.49 +33:48:36.2
17:08:18.90 +30:41:27.7
16:49:11.27 +34:05:49.8
17:07:11.02 +29:58:39.1
17:09:24.82 +30:44:45.5
17:04:54.56 +33:01:16.8
17:11:40.59 +32:53:35.0
17:08:58.11 +30:45:51.3
17:08:30.39 +30:46:17.1
16:46:29.13 +34:11:02.0
17:06:55.29 +33:04:25.0
17:06:30.81 +33:17:46.4
17:07:10.85 +33:19:39.7
17:09:27.77 +29:13:06.2
17:11:43.56 +33:05:11.4
17:11:25.83 +33:15:13.4
17:04:46.11 +33:54:06.9
17:07:33.52 +30:04:40.2
17:04:57.60 +33:19:49.2
17:07:44.43 +30:04:19.6
17:09:41.79 +33:17:50.4
17:12:13.94 +33:03:51.5
17:12:08.08 +33:06:06.5
17:09:00.51 +28:58:38.0
17:04:18.97 +33:36:25.8
17:05:01.17 +33:37:55.5
16:47:14.08 +33:57:01.5
17:12:51.96 +33:08:50.5
17:11:06.02 +32:55:02.9
17:09:44.12 +29:26:08.0
16:45:39.59 +33:23:43.6
17:09:35.66 +29:01:03.1
17:07:06.02 +33:17:01.5
17:06:54.15 +33:12:37.1
17:06:42.56 +33:07:19.6
17:11:28.51 +33:09:44.5
17:06:58.12 +30:01:17.6
17:05:03.04 +32:57:29.9
17:06:52.50 +30:01:20.3
17:08:26.43 +32:52:03.2
17:08:52.59 +29:00:53.4
17:08:45.76 +28:57:14.7
17:05:58.77 +33:18:36.1
17:11:56.32 +33:04:28.0
17:05:09.06 +33:40:36.0
17:06:52.54 +33:02:08.3
17:09:11.81 +32:29:34.4
17:04:06.59 +33:35:50.0
17:06:01.39 +33:20:25.7
17:06:17.78 +33:31:35.9
17:08:04.90 +29:28:13.4
17:08:51.14 +28:50:33.5
16:47:24.01 +34:06:33.3
17:02:20.65 +33:06:43.1
17:11:18.92 +33:09:56.5
17:08:49.14 +28:53:39.8
17:11:33.99 +33:36:56.4
17:08:43.44 +30:13:57.1
###################################################################################
17:04:28.50 +33:25:21.0 -- not an asteroid (will add it to exclusion list)
17:12:01.08 +32:54:16.1 -- not an asteroid (will add it to exclusion list)
17:11:14.18 +33:14:12.5 -- not an asteroid (will add it to exclusion list)
17:04:16.52 +33:28:27.0 -- not an asteroid (will add it to exclusion list)
17:11:22.77 +33:21:21.4 -- not an asteroid (will add it to exclusion list)
17:10:49.35 +33:23:53.6 -- not an asteroid (will add it to exclusion list)
17:12:39.43 +33:08:00.9 -- not an asteroid (will add it to exclusion list)
17:11:00.01 +33:39:18.1 -- not an asteroid (will add it to exclusion list)
17:09:24.98 +29:35:16.5 -- not an asteroid (will add it to exclusion list)
17:06:16.16 +33:31:06.0 -- not an asteroid (will add it to exclusion list)
17:11:45.53 +32:56:29.7 -- not an asteroid (will add it to exclusion list)
17:07:18.37 +33:14:52.7 -- not an asteroid (will add it to exclusion list)
17:08:25.97 +29:39:38.7 -- not an asteroid (will add it to exclusion list)
17:12:28.03 +33:05:40.4 -- not an asteroid (will add it to exclusion list)
17:12:19.66 +33:00:20.6 -- not an asteroid (will add it to exclusion list)
17:08:47.49 +30:47:13.1 -- not an asteroid (will add it to exclusion list)
17:05:24.43 +33:25:56.7 -- not an asteroid (will add it to exclusion list)
17:05:09.09 +33:26:06.4 -- not an asteroid (will add it to exclusion list)
17:07:25.55 +33:24:33.5 -- not an asteroid (will add it to exclusion list)
17:10:27.62 +33:15:55.4 -- not an asteroid (will add it to exclusion list)
17:08:22.78 +30:05:37.2 -- not an asteroid (will add it to exclusion list)
17:08:32.34 +30:01:35.5 -- not an asteroid (will add it to exclusion list)
17:09:18.29 +30:59:26.7 -- not an asteroid (will add it to exclusion list)
17:08:32.44 +30:41:57.9 -- not an asteroid (will add it to exclusion list)
17:04:09.66 +33:31:32.2 -- not an asteroid (will add it to exclusion list)
17:05:36.63 +33:25:16.0 -- not an asteroid (will add it to exclusion list)
17:02:09.67 +33:21:45.3 -- not an asteroid (will add it to exclusion list)
17:11:57.38 +32:51:28.7 -- not an asteroid (will add it to exclusion list)
17:08:24.22 +29:44:49.6 -- not an asteroid (will add it to exclusion list)
17:10:15.76 +31:06:12.2 -- not an asteroid (will add it to exclusion list)
17:09:05.78 +29:00:57.3 -- not an asteroid (will add it to exclusion list)
17:05:06.76 +33:23:58.8 -- not an asteroid (will add it to exclusion list)
17:05:53.26 +34:10:33.7 -- not an asteroid (will add it to exclusion list)
17:04:45.60 +33:03:03.3 -- not an asteroid (will add it to exclusion list)
16:47:12.06 +34:05:25.8 -- not an asteroid (will add it to exclusion list)
17:11:54.25 +33:00:21.5 -- not an asteroid (will add it to exclusion list)
17:11:03.11 +32:50:52.9 -- not an asteroid (will add it to exclusion list)
17:12:11.85 +33:01:53.6 -- not an asteroid (will add it to exclusion list)
17:09:07.25 +29:48:40.8 -- not an asteroid (will add it to exclusion list)
17:08:00.37 +30:12:15.5 -- not an asteroid (will add it to exclusion list)
17:08:50.75 +30:50:48.7 -- not an asteroid (will add it to exclusion list)
17:05:34.31 +33:14:07.2 -- not an asteroid (will add it to exclusion list)
17:10:11.23 +33:17:09.1 -- not an asteroid (will add it to exclusion list)
17:03:59.55 +33:40:18.9 -- not an asteroid (will add it to exclusion list)
17:11:24.30 +33:30:35.2 -- not an asteroid (will add it to exclusion list)
17:04:51.71 +33:48:07.4 -- not an asteroid (will add it to exclusion list)
17:09:16.92 +32:19:47.4 -- not an asteroid (will add it to exclusion list)
17:08:31.05 +28:44:41.8 -- not an asteroid (will add it to exclusion list)
17:10:13.17 +33:24:33.7 -- not an asteroid (will add it to exclusion list)
17:11:15.57 +33:08:46.1 -- not an asteroid (will add it to exclusion list)
17:08:56.84 +32:23:44.8 -- not an asteroid (will add it to exclusion list)
17:10:57.22 +32:41:11.6 -- not an asteroid (will add it to exclusion list)
17:07:03.59 +33:07:34.4 -- not an asteroid (will add it to exclusion list)
17:11:46.70 +33:03:22.5 -- not an asteroid (will add it to exclusion list)
17:05:17.62 +33:24:58.8 -- not an asteroid (will add it to exclusion list)
17:05:44.99 +33:00:31.9 -- not an asteroid (will add it to exclusion list)
16:47:04.36 +34:08:54.9 -- not an asteroid (will add it to exclusion list)
17:08:25.39 +30:41:12.9 -- not an asteroid (will add it to exclusion list)
17:11:43.70 +33:16:07.8 -- not an asteroid (will add it to exclusion list)
17:05:01.01 +33:32:19.0 -- not an asteroid (will add it to exclusion list)
17:04:58.22 +33:29:38.1 -- not an asteroid (will add it to exclusion list)
17:12:06.93 +33:13:21.4 -- not an asteroid (will add it to exclusion list)
17:08:34.43 +29:51:55.1 -- not an asteroid (will add it to exclusion list)
17:06:32.02 +33:18:42.1 -- not an asteroid (will add it to exclusion list)
17:05:59.49 +33:48:36.2 -- not an asteroid (will add it to exclusion list)
17:08:18.90 +30:41:27.7 -- not an asteroid (will add it to exclusion list)
16:49:11.27 +34:05:49.8 -- not an asteroid (will add it to exclusion list)
17:07:11.02 +29:58:39.1 -- not an asteroid (will add it to exclusion list)
17:09:24.82 +30:44:45.5 -- not an asteroid (will add it to exclusion list)
17:04:54.56 +33:01:16.8 -- not an asteroid (will add it to exclusion list)
17:11:40.59 +32:53:35.0 -- not an asteroid (will add it to exclusion list)
17:08:58.11 +30:45:51.3 -- not an asteroid (will add it to exclusion list)
17:08:30.39 +30:46:17.1 -- not an asteroid (will add it to exclusion list)
16:46:29.13 +34:11:02.0 -- not an asteroid (will add it to exclusion list)
17:06:55.29 +33:04:25.0 -- not an asteroid (will add it to exclusion list)
17:06:30.81 +33:17:46.4 -- not an asteroid (will add it to exclusion list)
17:07:10.85 +33:19:39.7 -- not an asteroid (will add it to exclusion list)
17:09:27.77 +29:13:06.2 -- not an asteroid (will add it to exclusion list)
17:11:43.56 +33:05:11.4 -- not an asteroid (will add it to exclusion list)
17:11:25.83 +33:15:13.4 -- not an asteroid (will add it to exclusion list)
17:04:46.11 +33:54:06.9 -- not an asteroid (will add it to exclusion list)
17:07:33.52 +30:04:40.2 -- not an asteroid (will add it to exclusion list)
17:04:57.60 +33:19:49.2 -- not an asteroid (will add it to exclusion list)
17:07:44.43 +30:04:19.6 -- not an asteroid (will add it to exclusion list)
17:09:41.79 +33:17:50.4 -- not an asteroid (will add it to exclusion list)
17:12:13.94 +33:03:51.5 -- not an asteroid (will add it to exclusion list)
17:12:08.08 +33:06:06.5 -- not an asteroid (will add it to exclusion list)
17:09:00.51 +28:58:38.0 -- not an asteroid (will add it to exclusion list)
17:04:18.97 +33:36:25.8 -- not an asteroid (will add it to exclusion list)
17:05:01.17 +33:37:55.5 -- not an asteroid (will add it to exclusion list)
16:47:14.08 +33:57:01.5 -- not an asteroid (will add it to exclusion list)
17:12:51.96 +33:08:50.5 -- not an asteroid (will add it to exclusion list)
17:11:06.02 +32:55:02.9 -- not an asteroid (will add it to exclusion list)
17:09:44.12 +29:26:08.0 -- not an asteroid (will add it to exclusion list)
16:45:39.59 +33:23:43.6 -- not an asteroid (will add it to exclusion list)
17:09:35.66 +29:01:03.1 -- not an asteroid (will add it to exclusion list)
17:07:06.02 +33:17:01.5 -- not an asteroid (will add it to exclusion list)
17:06:54.15 +33:12:37.1 -- not an asteroid (will add it to exclusion list)
17:06:42.56 +33:07:19.6 -- not an asteroid (will add it to exclusion list)
17:11:28.51 +33:09:44.5 -- not an asteroid (will add it to exclusion list)
17:06:58.12 +30:01:17.6 -- not an asteroid (will add it to exclusion list)
17:05:03.04 +32:57:29.9 -- not an asteroid (will add it to exclusion list)
17:06:52.50 +30:01:20.3 -- not an asteroid (will add it to exclusion list)
17:08:26.43 +32:52:03.2 -- not an asteroid (will add it to exclusion list)
17:08:52.59 +29:00:53.4 -- not an asteroid (will add it to exclusion list)
17:08:45.76 +28:57:14.7 -- not an asteroid (will add it to exclusion list)
17:05:58.77 +33:18:36.1 -- not an asteroid (will add it to exclusion list)
17:11:56.32 +33:04:28.0 -- not an asteroid (will add it to exclusion list)
17:05:09.06 +33:40:36.0 -- not an asteroid (will add it to exclusion list)
17:06:52.54 +33:02:08.3 -- not an asteroid (will add it to exclusion list)
17:09:11.81 +32:29:34.4 -- not an asteroid (will add it to exclusion list)
17:04:06.59 +33:35:50.0 -- not an asteroid (will add it to exclusion list)
17:06:01.39 +33:20:25.7 -- not an asteroid (will add it to exclusion list)
17:06:17.78 +33:31:35.9 -- not an asteroid (will add it to exclusion list)
17:08:04.90 +29:28:13.4 -- not an asteroid (will add it to exclusion list)
17:08:51.14 +28:50:33.5 -- not an asteroid (will add it to exclusion list)
16:47:24.01 +34:06:33.3 -- not an asteroid (will add it to exclusion list)
17:02:20.65 +33:06:43.1 -- not an asteroid (will add it to exclusion list)
17:11:18.92 +33:09:56.5 -- not an asteroid (will add it to exclusion list)
17:08:49.14 +28:53:39.8 -- not an asteroid (will add it to exclusion list)
17:11:33.99 +33:36:56.4 -- not an asteroid (will add it to exclusion list)
17:08:43.44 +30:13:57.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:45:39.59 +33:23:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:29.13 +34:11:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:04.36 +34:08:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:12.06 +34:05:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:14.08 +33:57:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:24.01 +34:06:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:11.27 +34:05:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:09.67 +33:21:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:20.65 +33:06:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:59.55 +33:40:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:06.59 +33:35:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:09.66 +33:31:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:16.52 +33:28:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:18.97 +33:36:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:28.50 +33:25:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:45.60 +33:03:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:46.11 +33:54:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:51.71 +33:48:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:54.56 +33:01:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:57.60 +33:19:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:58.22 +33:29:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:01.01 +33:32:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:01.17 +33:37:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:03.04 +32:57:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:06.76 +33:23:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:09.06 +33:40:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:09.09 +33:26:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:17.62 +33:24:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:24.43 +33:25:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:34.31 +33:14:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:36.63 +33:25:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:44.99 +33:00:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:53.26 +34:10:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:58.77 +33:18:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:59.49 +33:48:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:01.39 +33:20:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:16.16 +33:31:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:17.78 +33:31:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:30.81 +33:17:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:32.02 +33:18:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:42.56 +33:07:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:52.50 +30:01:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:52.54 +33:02:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:54.15 +33:12:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:55.29 +33:04:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:58.12 +30:01:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:03.59 +33:07:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:06.02 +33:17:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:10.85 +33:19:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:11.02 +29:58:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:18.37 +33:14:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:25.55 +33:24:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:33.52 +30:04:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:07:44.43 +30:04:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:00.37 +30:12:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:04.90 +29:28:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:18.90 +30:41:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:22.78 +30:05:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:24.22 +29:44:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:25.39 +30:41:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:25.97 +29:39:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:26.43 +32:52:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:30.39 +30:46:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:31.05 +28:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:32.34 +30:01:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:32.44 +30:41:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:34.43 +29:51:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:43.44 +30:13:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:45.76 +28:57:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:47.49 +30:47:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:49.14 +28:53:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:50.75 +30:50:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:51.14 +28:50:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:52.59 +29:00:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:56.84 +32:23:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:58.11 +30:45:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:00.51 +28:58:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:05.78 +29:00:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:07.25 +29:48:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:11.81 +32:29:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:16.92 +32:19:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:18.29 +30:59:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:24.82 +30:44:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:24.98 +29:35:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:27.77 +29:13:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:35.66 +29:01:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:41.79 +33:17:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:44.12 +29:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:11.23 +33:17:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:13.17 +33:24:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:15.76 +31:06:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:27.62 +33:15:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:49.35 +33:23:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:57.22 +32:41:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:00.01 +33:39:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:03.11 +32:50:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:06.02 +32:55:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:14.18 +33:14:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:15.57 +33:08:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:18.92 +33:09:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:22.77 +33:21:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:24.30 +33:30:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:25.83 +33:15:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:28.51 +33:09:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:33.99 +33:36:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:40.59 +32:53:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:43.56 +33:05:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:43.70 +33:16:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:45.53 +32:56:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:46.70 +33:03:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:54.25 +33:00:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:56.32 +33:04:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:57.38 +32:51:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:01.08 +32:54:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:06.93 +33:13:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:08.08 +33:06:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:11.85 +33:01:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:13.94 +33:03:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:19.66 +33:00:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:28.03 +33:05:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:39.43 +33:08:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:12:51.96 +33:08:50.5 -- 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)
16:45:39.59 +33:23:43.6 -- not a known variable star
16:46:29.13 +34:11:02.0 -- not a known variable star
16:47:04.36 +34:08:54.9 -- not a known variable star
16:47:12.06 +34:05:25.8 -- not a known variable star
16:47:14.08 +33:57:01.5 -- not a known variable star
16:47:24.01 +34:06:33.3 -- not a known variable star
16:49:11.27 +34:05:49.8 -- not a known variable star
17:02:09.67 +33:21:45.3 -- not a known variable star
17:02:20.65 +33:06:43.1 -- not a known variable star
17:03:59.55 +33:40:18.9 -- not a known variable star
17:04:06.59 +33:35:50.0 -- not a known variable star
17:04:09.66 +33:31:32.2 -- not a known variable star
17:04:16.52 +33:28:27.0 -- a known variable star
17:04:18.97 +33:36:25.8 -- not a known variable star
17:04:28.50 +33:25:21.0 -- not a known variable star
17:04:45.60 +33:03:03.3 -- not a known variable star
17:04:46.11 +33:54:06.9 -- not a known variable star
17:04:51.71 +33:48:07.4 -- a known variable star
17:04:54.56 +33:01:16.8 -- not a known variable star
17:04:57.60 +33:19:49.2 -- not a known variable star
17:04:58.22 +33:29:38.1 -- not a known variable star
17:05:01.01 +33:32:19.0 -- not a known variable star
17:05:01.17 +33:37:55.5 -- not a known variable star
17:05:03.04 +32:57:29.9 -- not a known variable star
17:05:06.76 +33:23:58.8 -- not a known variable star
17:05:09.06 +33:40:36.0 -- not a known variable star
17:05:09.09 +33:26:06.4 -- not a known variable star
17:05:17.62 +33:24:58.8 -- not a known variable star
17:05:24.43 +33:25:56.7 -- not a known variable star
17:05:34.31 +33:14:07.2 -- not a known variable star
17:05:36.63 +33:25:16.0 -- not a known variable star
17:05:44.99 +33:00:31.9 -- not a known variable star
17:05:53.26 +34:10:33.7 -- not a known variable star
17:05:58.77 +33:18:36.1 -- not a known variable star
17:05:59.49 +33:48:36.2 -- not a known variable star
17:06:01.39 +33:20:25.7 -- not a known variable star
17:06:16.16 +33:31:06.0 -- not a known variable star
17:06:17.78 +33:31:35.9 -- not a known variable star
17:06:30.81 +33:17:46.4 -- not a known variable star
17:06:32.02 +33:18:42.1 -- not a known variable star
17:06:42.56 +33:07:19.6 -- not a known variable star
17:06:52.50 +30:01:20.3 -- a known variable star
17:06:52.54 +33:02:08.3 -- not a known variable star
17:06:54.15 +33:12:37.1 -- not a known variable star
17:06:55.29 +33:04:25.0 -- not a known variable star
17:06:58.12 +30:01:17.6 -- not a known variable star
17:07:03.59 +33:07:34.4 -- not a known variable star
17:07:06.02 +33:17:01.5 -- not a known variable star
17:07:10.85 +33:19:39.7 -- not a known variable star
17:07:11.02 +29:58:39.1 -- not a known variable star
17:07:18.37 +33:14:52.7 -- not a known variable star
17:07:25.55 +33:24:33.5 -- not a known variable star
17:07:33.52 +30:04:40.2 -- not a known variable star
17:07:44.43 +30:04:19.6 -- not a known variable star
17:08:00.37 +30:12:15.5 -- not a known variable star
17:08:04.90 +29:28:13.4 -- not a known variable star
17:08:18.90 +30:41:27.7 -- not a known variable star
17:08:22.78 +30:05:37.2 -- not a known variable star
17:08:24.22 +29:44:49.6 -- not a known variable star
17:08:25.39 +30:41:12.9 -- not a known variable star
17:08:25.97 +29:39:38.7 -- not a known variable star
17:08:26.43 +32:52:03.2 -- not a known variable star
17:08:30.39 +30:46:17.1 -- not a known variable star
17:08:31.05 +28:44:41.8 -- not a known variable star
17:08:32.34 +30:01:35.5 -- not a known variable star
17:08:32.44 +30:41:57.9 -- not a known variable star
17:08:34.43 +29:51:55.1 -- not a known variable star
17:08:43.44 +30:13:57.1 -- not a known variable star
17:08:45.76 +28:57:14.7 -- not a known variable star
17:08:47.49 +30:47:13.1 -- not a known variable star
17:08:49.14 +28:53:39.8 -- not a known variable star
17:08:50.75 +30:50:48.7 -- not a known variable star
17:08:51.14 +28:50:33.5 -- not a known variable star
17:08:52.59 +29:00:53.4 -- not a known variable star
17:08:56.84 +32:23:44.8 -- not a known variable star
17:08:58.11 +30:45:51.3 -- not a known variable star
17:09:00.51 +28:58:38.0 -- not a known variable star
17:09:05.78 +29:00:57.3 -- not a known variable star
17:09:07.25 +29:48:40.8 -- not a known variable star
17:09:11.81 +32:29:34.4 -- not a known variable star
17:09:16.92 +32:19:47.4 -- not a known variable star
17:09:18.29 +30:59:26.7 -- not a known variable star
17:09:24.82 +30:44:45.5 -- not a known variable star
17:09:24.98 +29:35:16.5 -- a known variable star
17:09:27.77 +29:13:06.2 -- not a known variable star
17:09:35.66 +29:01:03.1 -- not a known variable star
17:09:41.79 +33:17:50.4 -- not a known variable star
17:09:44.12 +29:26:08.0 -- not a known variable star
17:10:11.23 +33:17:09.1 -- not a known variable star
17:10:13.17 +33:24:33.7 -- not a known variable star
17:10:15.76 +31:06:12.2 -- not a known variable star
17:10:27.62 +33:15:55.4 -- not a known variable star
17:10:49.35 +33:23:53.6 -- not a known variable star
17:10:57.22 +32:41:11.6 -- not a known variable star
17:11:00.01 +33:39:18.1 -- not a known variable star
17:11:03.11 +32:50:52.9 -- not a known variable star
17:11:06.02 +32:55:02.9 -- not a known variable star
17:11:14.18 +33:14:12.5 -- not a known variable star
17:11:15.57 +33:08:46.1 -- not a known variable star
17:11:18.92 +33:09:56.5 -- not a known variable star
17:11:22.77 +33:21:21.4 -- not a known variable star
17:11:24.30 +33:30:35.2 -- not a known variable star
17:11:25.83 +33:15:13.4 -- not a known variable star
17:11:28.51 +33:09:44.5 -- not a known variable star
17:11:33.99 +33:36:56.4 -- not a known variable star
17:11:40.59 +32:53:35.0 -- not a known variable star
17:11:43.56 +33:05:11.4 -- not a known variable star
17:11:43.70 +33:16:07.8 -- not a known variable star
17:11:45.53 +32:56:29.7 -- not a known variable star
17:11:46.70 +33:03:22.5 -- not a known variable star
17:11:54.25 +33:00:21.5 -- not a known variable star
17:11:56.32 +33:04:28.0 -- not a known variable star
17:11:57.38 +32:51:28.7 -- not a known variable star
17:12:01.08 +32:54:16.1 -- not a known variable star
17:12:06.93 +33:13:21.4 -- not a known variable star
17:12:08.08 +33:06:06.5 -- not a known variable star
17:12:11.85 +33:01:53.6 -- not a known variable star
17:12:13.94 +33:03:51.5 -- not a known variable star
17:12:19.66 +33:00:20.6 -- not a known variable star
17:12:28.03 +33:05:40.4 -- a known variable star
17:12:39.43 +33:08:00.9 -- a known variable star
17:12:51.96 +33:08:50.5 -- not a known variable star
Found 116 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
122 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 122 (excluding asteroids and hot pixels, 116 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)2461237.87467166 -observatory V36
07:16:32.26 +17:18:18.1 Mercury (4.8mag)
10:36:27.97 +09:58:20.9 Venus (-4.1mag)
04:42:01.93 +22:06:48.5 Mars (1.3mag)
08:22:09.64 +19:53:53.0 Jupiter (-1.8mag)
00:56:23.99 +03:22:06.8 Saturn (0.7mag)
04:08:20.93 +20:48:03.2 Uranus (5.8mag)
00:16:57.72 +00:19:56.1 Neptune (7.7mag)
20:30:21.17 -23:20:39.7 Pluto (14.4mag)
09:33:18.28 +14:40:12.9 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Jul 16 04:12 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461237.87467166:
08:22:08.79 +19:53:55.6 Io (6.0mag)
08:22:01.07 +19:54:26.6 Europa (6.3mag)
08:22:15.92 +19:53:33.3 Ganymede (5.6mag)
08:21:46.41 +19:55:19.0 Callisto (6.8mag)
08:20:25.11 +19:40:42.0 Himalia (15.7mag)
08:22:07.98 +19:54:00.3 Thebe (16.6mag)
08:19:45.88 +19:43:50.2 Elara (17.7mag)
08:25:52.45 +19:44:50.5 Pasiphae (17.9mag)
08:26:46.57 +19:59:52.0 Carme (19.0mag)
00:56:35.93 +03:21:52.7 Titan (8.5mag)
00:56:26.42 +03:21:51.9 Rhea (9.8mag)
00:55:49.20 +03:20:12.7 Iapetus (11.2mag)
00:56:10.59 +03:22:18.0 Hyperion (14.5mag)
00:56:16.65 +03:18:28.0 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 04:12 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.87467166:
17:54:54.09 -31:33:32.8 JWST
17:43:07.82 +34:36:51.1 Chandra
04:56:45.64 +48:40:55.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 04:12 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.87467166 -observatory V36
02:44:43.62 +15:07:44.3 17.8mag P/1996 R2 (Lagerkvist)
18:13:27.99 -34:30:30.9 13.8mag P/2010 H2 (Vales)
06:31:41.42 -68:14:45.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:52.44 +32:33:04.0 17.6mag C/2017 K2 (PANSTARRS)
02:19:23.52 +18:38:11.3 15.7mag P/2021 N1 (ZTF)
22:55:46.33 +32:15:00.2 17.3mag C/2022 E2 (ATLAS)
06:19:13.31 +26:52:05.1 16.7mag C/2022 N2 (PANSTARRS)
10:00:48.04 +29:30:36.0 16.9mag C/2022 QE78 (ATLAS)
09:13:38.82 +05:06:18.2 17.9mag C/2022 R6 (PANSTARRS)
18:03:37.63 +21:02:32.3 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.27 -11:32:03.3 17.8mag P/2023 B1 (PANSTARRS)
21:41:44.62 +67:32:10.9 17.8mag C/2023 H5 (Lemmon)
16:19:30.51 -10:42:11.1 14.0mag C/2023 R1 (PANSTARRS)
08:11:13.47 +66:02:25.0 17.9mag C/2024 A1 (ATLAS)
07:40:37.60 +30:18:13.5 14.8mag C/2024 E1 (Wierzchos)
15:13:34.88 +15:28:01.9 17.6mag C/2024 G6 (ATLAS)
19:33:30.53 +40:30:09.0 13.7mag C/2024 J3 (ATLAS)
21:41:04.67 +46:52:35.9 17.8mag C/2024 R4 (PANSTARRS)
04:55:16.76 -13:32:24.6 15.7mag C/2024 T5 (ATLAS)
06:39:30.07 +28:03:50.6 18.0mag C/2025 J1 (Borisov)
07:18:26.46 -13:26:47.8 16.8mag C/2025 R3 (PANSTARRS)
10:03:11.90 +22:10:05.6 17.6mag C/2025 V2 (Rankin)
12:46:46.36 +03:40:01.7 17.1mag C/2025 Y1 (ATLAS)
16:35:40.94 +79:09:28.9 17.2mag C/2026 A2 (Bok)
02:52:22.12 +45:29:30.9 16.8mag C/2026 B2 (Sun-Gao)
11:29:27.82 +05:34:04.2 17.0mag A/2026 E1
21:28:19.37 -17:20:42.2 7.1mag 10P/Tempel
11:16:21.31 -02:09:17.3 16.2mag 29P/Schwassmann-Wachmann
04:08:47.42 +30:11:59.1 17.9mag 47P/Ashbrook-Jackson
10:20:38.49 +12:05:02.2 17.1mag 63P/Wild
00:50:45.60 -05:02:51.4 15.5mag 65P/Gunn
04:41:56.39 +20:27:27.6 13.7mag 78P/Gehrels
02:31:50.01 +11:24:38.9 16.3mag 88P/Howell
06:53:18.44 +30:08:02.2 15.8mag 93P/Lovas
04:40:39.72 +31:18:31.5 16.7mag 114P/Wiseman-Skiff
08:23:24.72 +30:00:12.1 15.2mag 123P/West-Hartley
10:59:25.40 -01:15:21.5 16.9mag 124P/Mrkos
05:01:22.40 +20:58:11.8 16.2mag 128P/Shoemaker-Holt
05:47:33.88 +19:38:46.5 17.8mag 131P/Mueller
00:02:58.88 +03:08:58.2 17.9mag 139P/Vaisala-Oterma
07:35:13.41 +15:41:25.4 16.3mag 141P-D/Machholz
03:19:11.04 -20:37:32.4 15.2mag 161P/Hartley-IRAS
05:54:47.77 +35:09:41.8 15.4mag 162P/SidingSpring
18:46:30.26 +19:04:50.3 14.2mag 169P/NEAT
01:55:13.77 +08:13:59.2 17.6mag 220P/McNaught
16:35:30.06 -08:38:52.8 17.2mag 235P/LINEAR
08:57:54.96 +32:43:44.9 18.0mag 240P/NEAT
20:39:07.78 -50:48:23.4 17.8mag 259P/Garradd
02:16:14.81 +14:54:37.1 15.6mag 260P/McNaught
05:55:33.75 +37:16:37.6 17.4mag 295P/LINEAR
15:06:29.51 +05:30:22.1 17.6mag 391P/Kowalski
08:40:02.02 +19:25:39.1 17.9mag 450P/LONEOS
08:01:11.47 +38:42:45.4 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 04:12 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 16 04:12 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 16 04:12 tocp_transients_list.txt
############################################################
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 04:12 tns_transients_list.txt
