This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e
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 10.3261 2461231.8261 11.56 18:28:21.34 +43:03:26.6
71.23185 22.12926 galactic Lyr Second-epoch detections are separated by 1.1" and 5.5 pix
The object was found in VSX 2" NSVS J1828215+430325
Type: L:
# Max. Min./Amp. JD0 Period
11.322 R1 Y 0.689 R1 225.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:28:21.34 +43:03:26.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:28:21.34 +43:03:26.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1828215+430325,2461231.8261,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1828215+430325 20260710.3261 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.53 17:18:22.58 +46:08:09.8
72.00545 34.91465 galactic Her Second-epoch detections are separated by 2.3" and 5.9 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 | 17:18:22.58 +46:08:09.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.726+/-0.030 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:22.58 +46:08:09.8: 13.53 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:22.58 +46:08:09.8: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 18 22.58 +46 08 09.8 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,2461231.8261,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.37 17:20:23.26 +47:12:21.4
73.33521 34.64842 galactic Her Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J260.0970+47.2057 | 17:20:23.26 +47:12:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.273+/-0.032 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:23.26 +47:12:21.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:23.26 +47:12:21.4: 13.32 +/- 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 10.3261* 17 20 23.26 +47 12 21.4 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
ATO J260.0970+47.2057,2461231.8261,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.0970+47.2057 20260710.3261 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 10.3261 2461231.8261 12.05 17:23:40.54 +45:56:30.0
71.86564 33.98178 galactic Her Second-epoch detections are separated by 1.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J260.9235+45.9508 | 17:23:40.54 +45:56:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:40.54 +45:56:30.0: 12.95 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:40.54 +45:56:30.0: 12.97 +/- 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 10.3261* 17 23 40.54 +45 56 30.0 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 J260.9235+45.9508,2461231.8261,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.9235+45.9508 20260710.3261 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 10.3261 2461231.8261 12.65 18:19:11.81 +44:18:30.4
72.03798 24.06747 galactic Lyr Second-epoch detections are separated by 0.6" and 5.6 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 | 18:19:11.81 +44:18:30.4 (user input) | T | P | (position from user input) J-Ks=0.602+/-0.030 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:19:11.81 +44:18:30.4: 13.52 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:19:11.81 +44:18:30.4: 13.54 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.06 17:20:27.43 +45:58:50.6
71.85231 34.54236 galactic Her Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J260.1204+45.9799 | 17:20:27.43 +45:58:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.203+/-0.034 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:27.43 +45:58:50.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:27.43 +45:58:50.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 20 27.43 +45 58 50.6 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
ATO J260.1204+45.9799,2461231.8261,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.1204+45.9799 20260710.3261 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.07 18:19:51.90 +44:23:22.9
72.15814 23.97354 galactic Lyr Second-epoch detections are separated by 1.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:51.90 +44:23:22.9 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.251+/-0.032 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:19:51.90 +44:23:22.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:19:51.90 +44:23:22.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.09 17:22:55.77 +45:53:23.3
71.78869 34.10615 galactic Her Second-epoch detections are separated by 1.8" and 5.8 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 | 17:22:55.77 +45:53:23.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.350+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:55.77 +45:53:23.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:55.77 +45:53:23.3: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 22 55.77 +45 53 23.3 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,2461231.8261,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.40 17:19:36.45 +45:33:55.9
71.33437 34.65448 galactic Her Second-epoch detections are separated by 2.6" and 5.8 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 | 17:19:36.45 +45:33:55.9 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.035 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:36.45 +45:33:55.9: 13.31 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:36.45 +45:33:55.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 19 36.45 +45 33 55.9 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,2461231.8261,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.63 18:27:18.49 +45:18:37.1
73.51209 22.95123 galactic Lyr Second-epoch detections are separated by 1.3" and 5.6 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 J276.8308+45.3140 | 18:27:18.49 +45:18:37.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.319+/-0.033 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:18.49 +45:18:37.1: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:18.49 +45:18:37.1: 13.52 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J276.8308+45.3140,2461231.8261,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.8308+45.3140 20260710.3261 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 10.3261 2461231.8261 11.90 17:58:09.21 +41:25:40.5
67.89124 27.09494 galactic Her Second-epoch detections are separated by 2.2" and 6.0 pix
The object was found in VSX 1" FV Her
Type: SR
# Max. Min./Amp. JD0 Period
13.952 g Y 0.991 g 2458379.87130 144.749850000000
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:58:09.21 +41:25:40.5: 13.08 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:58:09.21 +41:25:40.5: 13.07 +/- 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 10.3261* 17 58 09.21 +41 25 40.5 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
FV Her,2461231.8261,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FV Her 20260710.3261 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.37 17:16:41.72 +45:30:54.3
71.22160 35.15847 galactic Her Second-epoch detections are separated by 2.4" and 6.6 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 | 17:16:41.72 +45:30:54.3 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.311+/-0.033 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:16:41.72 +45:30:54.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:16:41.72 +45:30:54.3: 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 10.3261* 17 16 41.72 +45 30 54.3 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,2461231.8261,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.51 17:23:00.92 +45:43:25.7
71.59082 34.07570 galactic Her Second-epoch detections are separated by 0.3" and 6.0 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 | 17:23:00.92 +45:43:25.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.447+/-0.033 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:00.92 +45:43:25.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:00.92 +45:43:25.7: 13.44 +/- 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 10.3261* 17 23 00.92 +45 43 25.7 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,2461231.8261,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.41 17:20:12.33 +45:15:04.9
70.96570 34.52183 galactic Her Second-epoch detections are separated by 1.5" and 6.0 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 | 17:20:12.33 +45:15:04.9 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.249+/-0.034 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:12.33 +45:15:04.9: 13.40 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:12.33 +45:15:04.9: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 10.3261* 17 20 12.33 +45 15 04.9 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,2461231.8261,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.66 18:21:13.57 +44:17:42.1
72.12889 23.71378 galactic Lyr Second-epoch detections are separated by 0.8" and 5.6 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 J275.3120+44.2948 | 18:21:13.57 +44:17:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.631+/-0.027 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:13.57 +44:17:42.1: 13.68 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:13.57 +44:17:42.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.3120+44.2948,2461231.8261,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.3120+44.2948 20260710.3261 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 11.89 17:20:26.33 +45:09:41.7
70.86188 34.47255 galactic Her Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:20:26.33 +45:09:41.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:26.33 +45:09:41.7: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:26.33 +45:09:41.7: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 10.3261* 17 20 26.33 +45 09 41.7 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,2461231.8261,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.39 17:53:20.83 +48:33:31.7
75.64464 29.30977 galactic Her Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:53:20.83 +48:33:31.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.687+/-0.030 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:53:20.83 +48:33:31.7: 13.21 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:53:20.83 +48:33:31.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 10.3261* 17 53 20.83 +48 33 31.7 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,2461231.8261,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.27 17:19:58.07 +45:57:15.3
71.81162 34.62488 galactic Her Second-epoch detections are separated by 3.1" and 5.6 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 | 17:19:58.07 +45:57:15.3 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.031 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:58.07 +45:57:15.3: 13.23 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:58.07 +45:57:15.3: 13.33 +/- 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 10.3261* 17 19 58.07 +45 57 15.3 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,2461231.8261,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.34 17:20:17.21 +45:39:01.5
71.44970 34.54352 galactic Her Second-epoch detections are separated by 1.6" and 6.1 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 | 17:20:17.21 +45:39:01.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.513+/-0.030 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:17.21 +45:39:01.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:17.21 +45:39:01.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 10.3261* 17 20 17.21 +45 39 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,2461231.8261,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 11.95 17:23:36.84 +45:57:07.7
71.87700 33.99343 galactic Her Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:23:36.84 +45:57:07.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.409+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:36.84 +45:57:07.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:36.84 +45:57:07.7: 12.87 +/- 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 10.3261* 17 23 36.84 +45 57 07.7 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,2461231.8261,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.54 18:33:18.17 +40:47:31.4
69.22009 20.55845 galactic Lyr Second-epoch detections are separated by 1.2" and 5.9 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 | 18:33:18.17 +40:47:31.4 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.028 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:33:18.17 +40:47:31.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:33:18.17 +40:47:31.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.50 17:23:32.74 +45:02:13.2
70.77773 33.91463 galactic Her Second-epoch detections are separated by 2.7" and 5.9 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 | 17:23:32.74 +45:02:13.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.459+/-0.035 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:32.74 +45:02:13.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:32.74 +45:02:13.2: 13.54 +/- 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 10.3261* 17 23 32.74 +45 02 13.2 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,2461231.8261,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.25 17:19:49.33 +45:32:24.9
71.30775 34.61483 galactic Her Second-epoch detections are separated by 1.4" and 6.4 pix
The object was found in VSX 1" Gaia DR3 1361664135034132992
Type: ROT
# Max. Min./Amp. JD0 Period
12.910 G 12.930 G G
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:49.33 +45:32:24.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:49.33 +45:32:24.9: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 19 49.33 +45 32 24.9 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 1361664135034132992,2461231.8261,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1361664135034132992 20260710.3261 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.53 18:27:14.80 +44:22:52.8
72.54093 22.70241 galactic Lyr Second-epoch detections are separated by 1.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:14.80 +44:22:52.8 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:14.80 +44:22:52.8: 13.43 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:14.80 +44:22:52.8: 13.47 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.43 17:19:02.75 +45:36:16.4
71.37143 34.75573 galactic Her Second-epoch detections are separated by 1.0" and 6.1 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 | 17:19:02.75 +45:36:16.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:02.75 +45:36:16.4: 13.43 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:02.75 +45:36:16.4: 13.41 +/- 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 10.3261* 17 19 02.75 +45 36 16.4 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,2461231.8261,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.58 17:20:29.49 +45:22:54.9
71.12905 34.48375 galactic Her Second-epoch detections are separated by 7.6" and 4.9 pix
The object was found in VSX 1" Gaia DR3 1361646955164922368
Type: ROT
# Max. Min./Amp. JD0 Period
13.470 G 13.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:29.49 +45:22:54.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:29.49 +45:22:54.9: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 10.3261* 17 20 29.49 +45 22 54.9 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
Gaia DR3 1361646955164922368,2461231.8261,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1361646955164922368 20260710.3261 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 10.3261 2461231.8261 12.69 18:27:16.13 +44:16:55.4
72.43893 22.67056 galactic Lyr Second-epoch detections are separated by 2.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:16.13 +44:16:55.4 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.033 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:16.13 +44:16:55.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:16.13 +44:16:55.4: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 11.89 17:21:11.95 +45:37:02.9
71.42716 34.38174 galactic Her Second-epoch detections are separated by 1.6" and 6.0 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 | 17:21:11.95 +45:37:02.9 (user input) | T | P | (position from user input) J-Ks=0.638+/-0.062 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:11.95 +45:37:02.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:11.95 +45:37:02.9: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 21 11.95 +45 37 02.9 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,2461231.8261,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.21 17:51:45.09 +50:31:24.3
77.83831 29.84559 galactic Dra Second-epoch detections are separated by 1.8" and 5.8 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 | 17:51:45.09 +50:31:24.3 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.032 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:51:45.09 +50:31:24.3: 13.15 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:51:45.09 +50:31:24.3: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.64 18:20:21.74 +44:31:16.3
72.32251 23.92253 galactic Lyr Second-epoch detections are separated by 1.2" and 5.8 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 | 18:20:21.74 +44:31:16.3 (user input) | T | P | (position from user input) J-Ks=0.259+/-0.036 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:20:21.74 +44:31:16.3: 13.66 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:20:21.74 +44:31:16.3: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.54 17:22:50.34 +46:46:50.3
72.85943 34.19944 galactic Her Second-epoch detections are separated by 2.7" and 5.6 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 | 17:22:50.34 +46:46:50.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:50.34 +46:46:50.3: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:50.34 +46:46:50.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 22 50.34 +46 46 50.3 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,2461231.8261,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.70 17:22:00.57 +45:52:30.9
71.75349 34.26426 galactic Her Second-epoch detections are separated by 2.6" and 5.7 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 | 17:22:00.57 +45:52:30.9 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:00.57 +45:52:30.9: 13.79 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:00.57 +45:52:30.9: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 10.3261* 17 22 00.57 +45 52 30.9 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,2461231.8261,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.54 17:20:33.11 +45:24:45.0
71.16717 34.47600 galactic Her Second-epoch detections are separated by 1.3" and 6.3 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 | 17:20:33.11 +45:24:45.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.383+/-0.034 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:33.11 +45:24:45.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:33.11 +45:24:45.0: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 20 33.11 +45 24 45.0 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,2461231.8261,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.29 17:20:37.84 +45:08:04.3
70.83309 34.43632 galactic Her Second-epoch detections are separated by 1.3" and 6.3 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 | 17:20:37.84 +45:08:04.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.513+/-0.031 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:37.84 +45:08:04.3: 13.38 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:37.84 +45:08:04.3: 13.52 +/- 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 10.3261* 17 20 37.84 +45 08 04.3 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,2461231.8261,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.47 17:20:25.86 +45:33:43.1
71.34547 34.51059 galactic Her Second-epoch detections are separated by 1.1" and 5.9 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 | 17:20:25.86 +45:33:43.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.471+/-0.031 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:25.86 +45:33:43.1: 13.57 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:25.86 +45:33:43.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 10.3261* 17 20 25.86 +45 33 43.1 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
target,2461231.8261,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.12 17:20:55.47 +45:22:18.4
71.12531 34.40710 galactic Her Second-epoch detections are separated by 1.5" and 5.9 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 | 17:20:55.47 +45:22:18.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.386+/-0.035 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:55.47 +45:22:18.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:55.47 +45:22:18.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 20 55.47 +45 22 18.4 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,2461231.8261,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.17 17:18:00.77 +44:37:31.4
70.16392 34.85008 galactic Her Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:18:00.77 +44:37:31.4 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:00.77 +44:37:31.4: 13.07 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:00.77 +44:37:31.4: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 18 00.77 +44 37 31.4 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,2461231.8261,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.09 17:20:25.64 +45:22:45.2
71.12455 34.49473 galactic Her Second-epoch detections are separated by 2.3" and 6.4 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 | 17:20:25.64 +45:22:45.2 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:25.64 +45:22:45.2: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:25.64 +45:22:45.2: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 10.3261* 17 20 25.64 +45 22 45.2 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,2461231.8261,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.13 18:21:12.68 +44:21:18.0
72.19124 23.73235 galactic Lyr Second-epoch detections are separated by 0.7" and 5.7 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 J275.3050+44.3576 | 18:21:12.68 +44:21:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.426+/-0.029 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:12.68 +44:21:18.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:12.68 +44:21:18.0: 13.07 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J275.3050+44.3576,2461231.8261,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J275.3050+44.3576 20260710.3261 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.28 17:20:31.35 +45:09:45.4
70.86480 34.45796 galactic Her Second-epoch detections are separated by 0.6" and 6.3 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 J260.1355+45.1634 | 17:20:31.35 +45:09:45.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.273+/-0.035 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:31.35 +45:09:45.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:31.35 +45:09:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 20 31.35 +45 09 45.4 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
ATO J260.1355+45.1634,2461231.8261,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.1355+45.1634 20260710.3261 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 10.3261 2461231.8261 12.44 18:27:30.46 +45:46:02.5
73.99993 23.04321 galactic Lyr Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:30.46 +45:46:02.5 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.032 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:30.46 +45:46:02.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:30.46 +45:46:02.5: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.32 17:20:12.32 +45:09:27.3
70.85237 34.51315 galactic Her Second-epoch detections are separated by 2.8" and 5.8 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 | 17:20:12.32 +45:09:27.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.700+/-0.029 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:12.32 +45:09:27.3: 13.33 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:12.32 +45:09:27.3: 13.29 +/- 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 10.3261* 17 20 12.32 +45 09 27.3 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,2461231.8261,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.58 17:54:20.42 +49:25:58.4
76.66364 29.28121 galactic Her Second-epoch detections are separated by 1.2" and 5.6 pix
The object was found in VSX 1" NSVS J1754204+492600
Type: SR
# Max. Min./Amp. JD0 Period
14.687 g Y 1.577 g 2458597.12650 153.402100700000
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:54:20.42 +49:25:58.4: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:54:20.42 +49:25:58.4: 13.48 +/- 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 10.3261* 17 54 20.42 +49 25 58.4 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
NSVS J1754204+492600,2461231.8261,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1754204+492600 20260710.3261 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 10.3261 2461231.8261 12.12 17:20:04.09 +45:31:53.1
71.30167 34.57115 galactic Her Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J260.0010+45.5287 | 17:20:04.09 +45:31:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.573+/-0.033 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:04.09 +45:31:53.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:04.09 +45:31:53.1: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 20 04.09 +45 31 53.1 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 J260.0010+45.5287,2461231.8261,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.0010+45.5287 20260710.3261 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 10.3261 2461231.8261 12.66 18:38:28.17 +44:03:40.8
72.85605 20.68766 galactic Lyr Second-epoch detections are separated by 2.0" and 5.9 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 | 18:38:28.17 +44:03:40.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.388+/-0.024 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:38:28.17 +44:03:40.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:38:28.17 +44:03:40.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.46 18:21:10.95 +44:31:47.6
72.37394 23.78385 galactic Lyr Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:10.95 +44:31:47.6 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.025 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:10.95 +44:31:47.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:10.95 +44:31:47.6: 13.36 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.38 17:23:05.87 +45:30:17.1
71.32932 34.04026 galactic Her Second-epoch detections are separated by 2.3" and 6.1 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 | 17:23:05.87 +45:30:17.1 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:05.87 +45:30:17.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:05.87 +45:30:17.1: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 23 05.87 +45 30 17.1 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,2461231.8261,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.38 18:28:43.22 +44:18:21.7
72.54387 22.42839 galactic Lyr Second-epoch detections are separated by 2.7" and 5.6 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 | 18:28:43.22 +44:18:21.7 (user input) | T | P | (position from user input) J-Ks=0.261+/-0.034 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:28:43.22 +44:18:21.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:28:43.22 +44:18:21.7: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.60 18:21:50.28 +44:25:51.4
72.30384 23.64478 galactic Lyr Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:50.28 +44:25:51.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.430+/-0.028 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:50.28 +44:25:51.4: 13.54 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:50.28 +44:25:51.4: 13.60 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.54 17:21:48.44 +45:41:04.1
71.51970 34.28201 galactic Her Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:21:48.44 +45:41:04.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:48.44 +45:41:04.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:48.44 +45:41:04.1: 13.46 +/- 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 10.3261* 17 21 48.44 +45 41 04.1 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
target,2461231.8261,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.37 17:16:54.76 +45:41:31.3
71.44096 35.13439 galactic Her Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:16:54.76 +45:41:31.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.328+/-0.030 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:16:54.76 +45:41:31.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:16:54.76 +45:41:31.3: 13.40 +/- 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 10.3261* 17 16 54.76 +45 41 31.3 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,2461231.8261,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.55 18:27:41.90 +44:17:59.4
72.48100 22.60189 galactic Lyr Second-epoch detections are separated by 0.2" and 5.7 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 | 18:27:41.90 +44:17:59.4 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.035 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:41.90 +44:17:59.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:41.90 +44:17:59.4: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.20 17:21:46.41 +45:40:03.7
71.49883 34.28636 galactic Her Second-epoch detections are separated by 1.0" and 6.3 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 | 17:21:46.41 +45:40:03.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.641+/-0.030 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:46.41 +45:40:03.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:46.41 +45:40:03.7: 13.22 +/- 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 10.3261* 17 21 46.41 +45 40 03.7 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,2461231.8261,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.04 18:37:48.48 +44:14:00.3
72.99141 20.85402 galactic Lyr Second-epoch detections are separated by 1.4" and 5.6 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 | 18:37:48.48 +44:14:00.3 (user input) | T | P | (position from user input) J-Ks=0.571+/-0.025 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:37:48.48 +44:14:00.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:37:48.48 +44:14:00.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 11.70 17:23:06.90 +45:53:23.8
71.79248 34.07402 galactic Her Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1361686739445372032 | 17:23:06.94 +45:53:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.363+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:06.90 +45:53:23.8: 12.60 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:06.90 +45:53:23.8: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 23 06.90 +45 53 23.8 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 1361686739445372032,2461231.8261,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1361686739445372032 20260710.3261 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 10.3261 2461231.8261 12.15 17:18:40.59 +45:39:55.1
71.43856 34.82515 galactic Her Second-epoch detections are separated by 2.9" and 6.0 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 1361712822783435520 | 17:18:39.11 +45:40:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.718+/-0.032 (K)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:40.59 +45:39:55.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:40.59 +45:39:55.1: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 10.3261* 17 18 40.59 +45 39 55.1 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
Gaia DR3 1361712822783435520,2461231.8261,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1361712822783435520 20260710.3261 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.41 17:38:32.88 +42:51:12.8
68.65415 30.94075 galactic Her Second-epoch detections are separated by 2.5" and 5.7 pix
The object was found in VSX 0" NSVS J1738327+425112
Type: SR
# Max. Min./Amp. JD0 Period
14.341 g Y 0.937 g 2458283.88000 97.335714600000
The object was not found in astcheck.
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:38:32.88 +42:51:12.8: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:38:32.88 +42:51:12.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3261* 17 38 32.88 +42 51 12.8 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
NSVS J1738327+425112,2461231.8261,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1738327+425112 20260710.3261 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 10.3261 2461231.8261 12.58 18:26:43.99 +44:23:50.3
72.52955 22.79493 galactic Lyr Second-epoch detections are separated by 0.3" and 5.6 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 | 18:26:43.99 +44:23:50.3 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.038 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:26:43.99 +44:23:50.3: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:26:43.99 +44:23:50.3: 13.58 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8261,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.03 17:54:41.41 +48:31:45.2
75.65098 29.08560 galactic Her Second-epoch detections are separated by 1.0" and 5.8 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 | 17:54:41.41 +48:31:45.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.251+/-0.034 (F)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:54:41.41 +48:31:45.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:54:41.41 +48:31:45.2: 12.89 +/- 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 10.3261* 17 54 41.41 +48 31 45.2 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,2461231.8261,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3261 2461231.8261 12.38 17:20:20.33 +45:37:07.1
71.41224 34.53167 galactic Her Second-epoch detections are separated by 2.0" and 5.8 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 | 17:20:20.33 +45:37:07.1 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.031 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:20.33 +45:37:07.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:20.33 +45:37:07.1: 13.37 +/- 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 10.3261* 17 20 20.33 +45 37 07.1 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,2461231.8261,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 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 10.3261 2461231.8261 12.01 17:21:12.47 +45:21:17.9
71.11067 34.35598 galactic Her Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:21:12.47 +45:21:17.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.338+/-0.033 (G)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:12.47 +45:21:17.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:12.47 +45:21:17.9: 12.96 +/- 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 10.3261* 17 21 12.47 +45 21 17.9 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
target,2461231.8261,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3261 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461172.84898253 12.05.2026 08:22:22.091 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
First image: 2461172.84898253 12.05.2026 08:22:22.091 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Last image: 2461231.82640900 10.07.2026 07:49:51.738 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 10 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): 17034
Objects passed selection criteria: 16971
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 10887.8
Average stars matched: 10421.5 (95.7177 %)
Memory usage VmPeak: 122024 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:12:39 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: 2461172.84898253 12.05.2026 08:22:22.091 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
First image: 2461172.84898253 12.05.2026 08:22:22.091 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Last image: 2461231.82640900 10.07.2026 07:49:51.738 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 150
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.12
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: 131 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): 91298
Objects passed selection criteria: 91008
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 63193.8
Average stars matched: 60295.2 (95.4133 %)
Memory usage VmPeak: 1985960 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:18:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
SExtractor catalog cache: saved Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.cat to cache
SExtractor catalog cache: saved Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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: 2461231.82585091
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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits exists and is non-empty
Saving wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits to local_wcs_cache/
'wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits' -> 'local_wcs_cache/wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits'
wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits exists and is non-empty
Saving wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits to local_wcs_cache/
'wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits' -> 'local_wcs_cache/wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits'
wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits exists and is non-empty
Saving wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits to local_wcs_cache/
'wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits' -> 'local_wcs_cache/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits'
wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits exists and is non-empty
Saving wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits to local_wcs_cache/
'wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits' -> 'local_wcs_cache/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits (1st reference image)
verification OK: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:00:01.525 +46:01:06.10 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-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits (1st new image)
verification OK: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:00:00.556 +45:58:18.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:01.525 +46:01:06.10
Second-epoch image center 18:00:00.556 +45:58:18.73
Angular distance between the image centers 0.0466 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits (2nd new image)
verification OK: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:59:58.646 +45:58:46.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:00:01.525 +46:01:06.10
Second-epoch image center 17:59:58.646 +45:58:46.20
Angular distance between the image centers 0.0397 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 18:00:00.556 +45:58:18.73
Second-epoch second image center 17:59:58.646 +45:58:46.20
Angular distance between the image centers 0.00942 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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits &> /tmp/tmp.7fcdT9fOKk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits &> /tmp/tmp.5ZpbRKr0hT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits &> /tmp/tmp.WESaKKNgiD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits &> /tmp/tmp.fPjm70CKm0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
Found non-empty wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
The reference image (wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits) and catalog (wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat) found
'wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat' -> 'wcsmag.cat'
Read 17892 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.7111 to 282.2550 deg, Dec +40.3262 to +51.2744 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 257.7111 to 282.2550 deg, Dec 40.3262 to 51.2744 deg
Loaded 10597 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): 7786 out of 8250 total matches.
Matched with Tycho-2 8250 out of 17892 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.792950
a=0.000000 b=1.000000 c=22.792950
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 17892 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.7111 to 282.2550 deg, Dec +40.3262 to +51.2744 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 257.7111 to 282.2550 deg, Dec 40.3262 to 51.2744 deg
Loaded 10597 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): 7786 out of 8250 total matches.
Matched with Tycho-2 8250 out of 17892 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits:
Forced-photometry filter: calibrated wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits -> calib.txt_param_ref_wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits (aperture=6.4)
Read 18743 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.8587 to 282.3927 deg, Dec +40.2385 to +51.2513 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 257.8587 to 282.3927 deg, Dec 40.2385 to 51.2513 deg
Loaded 10714 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): 7784 out of 8275 total matches.
Matched with Tycho-2 8275 out of 18743 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits:
Forced-photometry filter: calibrated wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits -> calib.txt_param_ref_wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
2.3 pix Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
2.6 pix fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
2.6 pix fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
2.4 pix wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
2.3 pix wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Limiting magnitude estimates:
15.4 mag. Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
15.4 mag. Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
12.8 mag. fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
12.9 mag. fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.5 (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.7fcdT9fOKk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits' -> 'wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS_IMAGE_NAME=wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS-calibrated image found: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Checking if the catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits alredy exist and is non-empty...
Catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS catalog name: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1141, bad_region=0, passed=17892
Got 17892 stars (including 16735 good ones) from the SExtractor catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
util/solve_plate_with_UCAC5 got 17892 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 17651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 17651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 17651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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=Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits N_match=964 sigma_overall_arcsec=0.574 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.696 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.679 n_q1=206 n_q2=291 n_q3=198 n_q4=269 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits -region wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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.5ZpbRKr0hT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits' -> 'wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS_IMAGE_NAME=wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS-calibrated image found: wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Checking if the catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits alredy exist and is non-empty...
Catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS catalog name: wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1250, bad_region=0, passed=18743
Got 18743 stars (including 17481 good ones) from the SExtractor catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat
util/solve_plate_with_UCAC5 got 18743 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 651 to 708 (Dec 40.2 to 51.3)
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: 960 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 18384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 651 to 708 (Dec 40.2 to 51.3)
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(), 18386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 18385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits N_match=960 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.464 sigma_q4_arcsec=0.593 n_q1=251 n_q2=228 n_q3=234 n_q4=247 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits -region wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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.WESaKKNgiD (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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS_IMAGE_NAME=wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS-calibrated image found: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Checking if the catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS catalog name: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=96, bad_region=0, passed=3428
Got 3428 stars (including 3327 good ones) from the SExtractor catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 3428 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 3385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits N_match=955 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.344 n_q1=243 n_q2=179 n_q3=297 n_q4=236 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits -region wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.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.fPjm70CKm0 (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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS_IMAGE_NAME=wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS-calibrated image found: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Checking if the catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS catalog name: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=127, bad_region=0, passed=3736
Got 3736 stars (including 3600 good ones) from the SExtractor catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat
util/solve_plate_with_UCAC5 got 3736 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits N_match=955 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.399 n_q1=255 n_q2=171 n_q3=277 n_q4=252 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits -region wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits sigma_overall=0.574 worst_q_ratio=1.213
ref2=Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits sigma_overall=0.492 worst_q_ratio=1.204
new1=fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits sigma_overall=0.328 worst_q_ratio=1.213
new2=fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits sigma_overall=0.381 worst_q_ratio=1.117
reference average sigma_overall=0.533 worst_q_ratio=1.2085
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330_astrometric_residuals.png (964 matched stars from wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263_astrometric_residuals.png (960 matched stars from wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290_astrometric_residuals.png (955 matched stars from wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291_astrometric_residuals.png (955 matched stars from wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits'
Saving fully-calibrated image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits'
Preparing the HTML report for the field Her-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10002_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 10002_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:24:30.14 +46:08:05.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Her-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
SExtractor catalog cache: saved Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.cat to cache
SExtractor catalog cache: saved Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Creating symlink local_wcs_cache/wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Creating symlink local_wcs_cache/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Creating symlink local_wcs_cache/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits exists and is non-empty
wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits exists and is non-empty
wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits exists and is non-empty
wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits (1st reference image)
verification OK: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:00:01.525 +46:01:06.10 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-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits (1st new image)
verification OK: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:00:00.556 +45:58:18.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:01.525 +46:01:06.10
Second-epoch image center 18:00:00.556 +45:58:18.73
Angular distance between the image centers 0.0466 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits (2nd new image)
verification OK: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:59:58.646 +45:58:46.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:00:01.525 +46:01:06.10
Second-epoch image center 17:59:58.646 +45:58:46.20
Angular distance between the image centers 0.0397 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 18:00:00.556 +45:58:18.73
Second-epoch second image center 17:59:58.646 +45:58:46.20
Angular distance between the image centers 0.00942 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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits &> /tmp/tmp.K8hUF3GE4B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits &> /tmp/tmp.fgGCU1G3CC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits &> /tmp/tmp.KbALzHAB84
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits &> /tmp/tmp.li08cJJM4I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
Found non-empty wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits and wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
The reference image (wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits) and catalog (wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat) found
'wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat' -> 'wcsmag.cat'
Read 101201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.6725 to 282.3371 deg, Dec +40.3187 to +51.2824 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 257.6725 to 282.3371 deg, Dec 40.3187 to 51.2824 deg
Loaded 10665 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): 6872 out of 8285 total matches.
Matched with Tycho-2 8285 out of 101201 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.679200
a=0.000000 b=1.000000 c=22.679200
From vast_summary.log: estimated ref. image limiting mag.: -7.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 101201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.6725 to 282.3371 deg, Dec +40.3187 to +51.2824 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 257.6725 to 282.3371 deg, Dec 40.3187 to 51.2824 deg
Loaded 10665 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): 6872 out of 8285 total matches.
Matched with Tycho-2 8285 out of 101201 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits:
Forced-photometry filter: calibrated wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits -> calib.txt_param_ref_wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits (aperture=5.0)
Read 101702 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 257.7841 to 282.3947 deg, Dec +40.2385 to +51.2554 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 257.7841 to 282.3947 deg, Dec 40.2385 to 51.2554 deg
Loaded 10743 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): 6793 out of 8287 total matches.
Matched with Tycho-2 8287 out of 101702 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits:
Forced-photometry filter: calibrated wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits -> calib.txt_param_ref_wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 108 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
2.2 pix Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
2.5 pix fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
2.5 pix fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
2.2 pix wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
2.2 pix wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Limiting magnitude estimates:
15.6 mag. Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
15.6 mag. Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
13.1 mag. fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
13.1 mag. fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.8 (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.K8hUF3GE4B (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits' -> 'wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS_IMAGE_NAME=wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS-calibrated image found: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
Checking if the catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits alredy exist and is non-empty...
Catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits
WCS catalog name: wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=8193, bad_region=0, passed=101155
Got 101155 stars (including 92834 good ones) from the SExtractor catalog wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat
util/solve_plate_with_UCAC5 got 101155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 99816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 99814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 99814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits N_match=962 sigma_overall_arcsec=0.574 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.670 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.627 n_q1=205 n_q2=288 n_q3=195 n_q4=274 worst_quadrant_to_overall_ratio=1.166
The image catalog is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits -region wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.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.fgGCU1G3CC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits' -> 'wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS_IMAGE_NAME=wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS-calibrated image found: wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
Checking if the catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits alredy exist and is non-empty...
Catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat corresponding to the image wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits
WCS catalog name: wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=8586, bad_region=0, passed=101676
Got 101676 stars (including 92945 good ones) from the SExtractor catalog wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat
util/solve_plate_with_UCAC5 got 101676 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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 100218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 100218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 100218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits N_match=962 sigma_overall_arcsec=0.493 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.485 sigma_q4_arcsec=0.601 n_q1=254 n_q2=225 n_q3=243 n_q4=240 worst_quadrant_to_overall_ratio=1.219
The image catalog is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits -region wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.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.KbALzHAB84 (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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS_IMAGE_NAME=wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS-calibrated image found: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Checking if the catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
WCS catalog name: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=504, bad_region=10, passed=25233
Got 25233 stars (including 24676 good ones) from the SExtractor catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 25233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 24964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 24965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 24965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits N_match=954 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.284 sigma_q4_arcsec=0.318 n_q1=244 n_q2=174 n_q3=302 n_q4=234 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits -region wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.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.li08cJJM4I (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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS_IMAGE_NAME=wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS-calibrated image found: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Checking if the catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat corresponding to the image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
WCS catalog name: wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=580, bad_region=14, passed=26562
Got 26562 stars (including 25916 good ones) from the SExtractor catalog wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat
util/solve_plate_with_UCAC5 got 26562 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 26350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 26350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 26349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits N_match=953 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.379 n_q1=256 n_q2=167 n_q3=279 n_q4=251 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits -region wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-03_20.00sec_0.00C_LIGHTs_0290.fits
Saving fully-calibrated image wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.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_2026-07-10_CI_Her-02-Q1b1x1_030354_TTUQ1b1x1_2596207_B25bpO9e/wcs_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291.fits
Preparing the HTML report for the field Her-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:29:03.15 +48:12:37.7: 10.51 +/- 0.00 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:58:41.52 +45:29:58.3: 12.32 +/- 0.01 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:37:32.42 +44:57:39.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:17:06.02 +45:39:25.8: 11.79 +/- 0.01 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:00:55.43 +47:24:21.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:34:59.39 +41:04:42.6: 12.61 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:38:00.42 +43:36:56.4: 12.57 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:58:41.52 +45:29:58.3: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:00:55.43 +47:24:21.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:34:59.39 +41:04:42.6: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:17:06.02 +45:39:25.8: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 17:58:41.52 +45:29:58.3: ref_mag=12.33 +/- 0.01 new_mean_mag=12.4100 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:37:32.42 +44:57:39.6: 12.55 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 18:34:59.39 +41:04:42.6: ref_mag=12.57 +/- 0.01 new_mean_mag=12.1724 delta=0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:00:55.43 +47:24:21.0: ref_mag=12.76 +/- 0.01 new_mean_mag=12.3562 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter REJECTED candidate at 17:17:06.02 +45:39:25.8: ref_mag=11.83 +/- 0.01 new_mean_mag=11.2198 delta=0.61 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:37:32.42 +44:57:39.6: ref_mag=12.63 +/- 0.01 new_mean_mag=12.2646 delta=0.36 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:29:03.15 +48:12:37.7: 10.48 +/- 0.00 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:38:00.42 +43:36:56.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.00
Forced photometry filter REJECTED candidate at 18:29:03.15 +48:12:37.7: ref_mag=10.50 +/- 0.00 new_mean_mag=10.8295 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 17:38:00.42 +43:36:56.4: ref_mag=12.59 +/- 0.01 new_mean_mag=12.2628 delta=0.32 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:23.26 +47:12:21.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:28:21.34 +43:03:26.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:22.58 +46:08:09.8: 13.53 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:28:21.34 +43:03:26.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 18:28:21.34 +43:03:26.6: ref_mag=12.67 +/- 0.01 new_mean_mag=11.5284 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:22.58 +46:08:09.8: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:23.26 +47:12:21.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 17:18:22.58 +46:08:09.8: ref_mag=13.51 +/- 0.03 new_mean_mag=12.5100 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:23.26 +47:12:21.4: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3595 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:55.77 +45:53:23.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:40.54 +45:56:30.0: 12.95 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:27.43 +45:58:50.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:19:11.81 +44:18:30.4: 13.52 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:36.45 +45:33:55.9: 13.31 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:19:51.90 +44:23:22.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:27.43 +45:58:50.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:40.54 +45:56:30.0: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:27.43 +45:58:50.6: ref_mag=12.98 +/- 0.02 new_mean_mag=12.0456 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 17:23:40.54 +45:56:30.0: ref_mag=12.96 +/- 0.01 new_mean_mag=12.0197 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:36.45 +45:33:55.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:36.45 +45:33:55.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4016 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:19:11.81 +44:18:30.4: 13.54 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:55.77 +45:53:23.3: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter KEPT candidate at 18:19:11.81 +44:18:30.4: ref_mag=13.53 +/- 0.02 new_mean_mag=12.5984 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 17:22:55.77 +45:53:23.3: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0853 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:19:51.90 +44:23:22.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 18:19:51.90 +44:23:22.9: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0706 delta=0.90 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:20:06.95 +44:21:38.2: 13.30 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:20:06.95 +44:21:38.2: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter REJECTED candidate at 18:20:06.95 +44:21:38.2: ref_mag=13.29 +/- 0.02 new_mean_mag=12.4190 delta=0.88 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:18.49 +45:18:37.1: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:18.49 +45:18:37.1: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 18:27:18.49 +45:18:37.1: ref_mag=13.55 +/- 0.02 new_mean_mag=12.6266 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:58:09.21 +41:25:40.5: 13.08 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:58:09.21 +41:25:40.5: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 17:58:09.21 +41:25:40.5: ref_mag=13.07 +/- 0.01 new_mean_mag=11.9006 delta=1.17 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:16:41.72 +45:30:54.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:16:41.72 +45:30:54.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 17:16:41.72 +45:30:54.3: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3621 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:00.92 +45:43:25.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:00.92 +45:43:25.7: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 17:23:00.92 +45:43:25.7: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4696 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:12.33 +45:15:04.9: 13.40 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:13.57 +44:17:42.1: 13.68 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:12.33 +45:15:04.9: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:12.33 +45:15:04.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4136 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:26.33 +45:09:41.7: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:13.57 +44:17:42.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 18:21:13.57 +44:17:42.1: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6646 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:26.33 +45:09:41.7: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 17:20:26.33 +45:09:41.7: ref_mag=12.89 +/- 0.01 new_mean_mag=11.8936 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:53:20.83 +48:33:31.7: 13.21 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:58.07 +45:57:15.3: 13.23 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:53:20.83 +48:33:31.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 17:53:20.83 +48:33:31.7: ref_mag=13.25 +/- 0.02 new_mean_mag=12.3156 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:17.21 +45:39:01.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:58.07 +45:57:15.3: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:58.07 +45:57:15.3: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2609 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:17.21 +45:39:01.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:17.21 +45:39:01.5: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2918 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:36.84 +45:57:07.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:33:18.17 +40:47:31.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:36.84 +45:57:07.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 17:23:36.84 +45:57:07.7: ref_mag=12.86 +/- 0.01 new_mean_mag=11.9266 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:33:18.17 +40:47:31.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 18:33:18.17 +40:47:31.4: ref_mag=13.45 +/- 0.03 new_mean_mag=12.5320 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:32.74 +45:02:13.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:32.74 +45:02:13.2: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:23:32.74 +45:02:13.2: ref_mag=13.50 +/- 0.02 new_mean_mag=12.4680 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:49.33 +45:32:24.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:49.33 +45:32:24.9: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:49.33 +45:32:24.9: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2537 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:14.80 +44:22:52.8: 13.43 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:14.80 +44:22:52.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 18:27:14.80 +44:22:52.8: ref_mag=13.45 +/- 0.02 new_mean_mag=12.5258 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:19:02.75 +45:36:16.4: 13.43 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:19:02.75 +45:36:16.4: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:02.75 +45:36:16.4: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4119 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:29.49 +45:22:54.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:11.95 +45:37:02.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:16.13 +44:16:55.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:51:45.09 +50:31:24.3: 13.15 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:29.49 +45:22:54.9: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 17:20:29.49 +45:22:54.9: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5664 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:11.95 +45:37:02.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:16.13 +44:16:55.4: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 17:21:11.95 +45:37:02.9: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8879 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 18:27:16.13 +44:16:55.4: ref_mag=13.61 +/- 0.02 new_mean_mag=12.6843 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:51:45.09 +50:31:24.3: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 17:51:45.09 +50:31:24.3: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1773 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:20:21.74 +44:31:16.3: 13.66 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:20:21.74 +44:31:16.3: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.02
Forced photometry filter KEPT candidate at 18:20:21.74 +44:31:16.3: ref_mag=13.68 +/- 0.02 new_mean_mag=12.6090 delta=1.07 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:50.34 +46:46:50.3: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:50.34 +46:46:50.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 17:22:50.34 +46:46:50.3: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4595 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:22:00.57 +45:52:30.9: 13.79 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:33.11 +45:24:45.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:22:00.57 +45:52:30.9: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 17:22:00.57 +45:52:30.9: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7006 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:33.11 +45:24:45.0: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 17:20:33.11 +45:24:45.0: ref_mag=13.70 +/- 0.03 new_mean_mag=12.5408 delta=1.16 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:37.84 +45:08:04.3: 13.38 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:37.84 +45:08:04.3: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:37.84 +45:08:04.3: ref_mag=13.45 +/- 0.02 new_mean_mag=12.2674 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:25.86 +45:33:43.1: 13.57 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:25.86 +45:33:43.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 17:20:25.86 +45:33:43.1: ref_mag=13.58 +/- 0.03 new_mean_mag=12.4588 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:55.47 +45:22:18.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:12.68 +44:21:18.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:25.64 +45:22:45.2: 13.05 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:00.77 +44:37:31.4: 13.07 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:55.47 +45:22:18.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:55.47 +45:22:18.4: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1316 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:25.64 +45:22:45.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:12.68 +44:21:18.0: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:25.64 +45:22:45.2: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0909 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 18:21:12.68 +44:21:18.0: ref_mag=13.06 +/- 0.01 new_mean_mag=12.1385 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:00.77 +44:37:31.4: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 17:18:00.77 +44:37:31.4: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1275 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:31.35 +45:09:45.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:31.35 +45:09:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:31.35 +45:09:45.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2792 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:30.46 +45:46:02.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:30.46 +45:46:02.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 18:27:30.46 +45:46:02.5: ref_mag=13.36 +/- 0.02 new_mean_mag=12.4383 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:12.32 +45:09:27.3: 13.33 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:54:20.42 +49:25:58.4: 13.55 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:12.32 +45:09:27.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:12.32 +45:09:27.3: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3027 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:54:20.42 +49:25:58.4: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 17:54:20.42 +49:25:58.4: ref_mag=13.51 +/- 0.02 new_mean_mag=12.5777 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:38:28.17 +44:03:40.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:04.09 +45:31:53.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:38:28.17 +44:03:40.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 18:38:28.17 +44:03:40.8: ref_mag=13.65 +/- 0.03 new_mean_mag=12.6207 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:04.09 +45:31:53.1: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:04.09 +45:31:53.1: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1101 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:10.95 +44:31:47.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:05.87 +45:30:17.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:28:43.22 +44:18:21.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:10.95 +44:31:47.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 18:21:10.95 +44:31:47.6: ref_mag=13.33 +/- 0.02 new_mean_mag=12.4053 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:05.87 +45:30:17.1: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 17:23:05.87 +45:30:17.1: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3727 delta=0.91 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:28:43.22 +44:18:21.7: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 18:28:43.22 +44:18:21.7: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3695 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:21:50.28 +44:25:51.4: 13.54 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:48.44 +45:41:04.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:21:50.28 +44:25:51.4: 13.60 +/- 0.04 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:48.44 +45:41:04.1: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 18:21:50.28 +44:25:51.4: ref_mag=13.57 +/- 0.02 new_mean_mag=12.5795 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 17:21:48.44 +45:41:04.1: ref_mag=13.50 +/- 0.02 new_mean_mag=12.5182 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:16:54.76 +45:41:31.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:16:54.76 +45:41:31.3: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 17:16:54.76 +45:41:31.3: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3503 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:27:41.90 +44:17:59.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:27:41.90 +44:17:59.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 18:27:41.90 +44:17:59.4: ref_mag=13.50 +/- 0.02 new_mean_mag=12.5547 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:46.41 +45:40:03.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:46.41 +45:40:03.7: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 17:21:46.41 +45:40:03.7: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1547 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:37:48.48 +44:14:00.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:37:48.48 +44:14:00.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 18:37:48.48 +44:14:00.3: ref_mag=12.93 +/- 0.02 new_mean_mag=12.0128 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:23:06.90 +45:53:23.8: 12.60 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:23:06.90 +45:53:23.8: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 17:23:06.90 +45:53:23.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6890 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:18:40.59 +45:39:55.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:38:32.88 +42:51:12.8: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:18:40.59 +45:39:55.1: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 17:18:40.59 +45:39:55.1: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0715 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:38:32.88 +42:51:12.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 17:38:32.88 +42:51:12.8: ref_mag=13.40 +/- 0.02 new_mean_mag=12.4182 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 18:26:43.99 +44:23:50.3: 13.50 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 18:26:43.99 +44:23:50.3: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter KEPT candidate at 18:26:43.99 +44:23:50.3: ref_mag=13.53 +/- 0.02 new_mean_mag=12.5808 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:54:41.41 +48:31:45.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:20:20.33 +45:37:07.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:54:41.41 +48:31:45.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 17:54:41.41 +48:31:45.2: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9756 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:20:20.33 +45:37:07.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 17:20:20.33 +45:37:07.1: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3524 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:51.90 +46:03:11.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:51.90 +46:03:11.6: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 17:21:51.90 +46:03:11.6: ref_mag=13.02 +/- 0.02 new_mean_mag=12.3850 delta=0.63 (need > 0.90)
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-12_03-22-22_20.00sec_-4.90C_LIGHT_0330.fits at 17:21:12.47 +45:21:17.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-02-Q1b1x1_2026-05-14_05-06-58_20.00sec_-5.00C_LIGHT_0263.fits at 17:21:12.47 +45:21:17.9: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 17:21:12.47 +45:21:17.9: ref_mag=12.94 +/- 0.01 new_mean_mag=12.0096 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out03116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99574.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 113s
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: 62s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121672_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 121672_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 18:25:51.03 +45:37:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121675_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 121675_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121676_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 121676_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121677_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 121677_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 18:40:51.98 +47:06:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122082_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122082_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122085_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122085_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122137_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122137_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122182_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122182_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122219_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122219_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122224_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 122224_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:36:34.05 +48:33:26.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24127_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 24127_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58584_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 58584_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99574_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 99574_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55423_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 55423_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35941_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 35941_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56466_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 56466_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36828_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 36828_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55104_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 55104_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26375_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 26375_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:18:30.16 +43:01:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52479_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52479_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51957_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 51957_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:23:32.39 +45:35:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69210_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 69210_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:47:10.47 +50:29:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36545_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 36545_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47804_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 47804_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:21:09.95 +45:09:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47335_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 47335_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44627_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 44627_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:23:08.47 +44:52:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06083_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 06083_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52679_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52679_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53359_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53359_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49062_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 49062_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35993_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 35993_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48045_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 48045_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90678_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 90678_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56287_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 56287_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53185_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53185_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05813_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 05813_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:56.49 +40:59:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07516_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 07516_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:38.62 +41:09:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06337_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 06337_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:13.35 +41:01:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25234_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 25234_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:28.55 +42:56:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11578_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 11578_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:24:15.55 +41:39:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55546_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 55546_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03116_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 03116_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46193_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 46193_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27055_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 27055_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:48.44 +43:07:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28562_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 28562_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:18:19.49 +43:13:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52136_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52136_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36943_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 36943_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:59.27 +44:04:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37702_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 37702_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53039_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53039_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50351_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 50351_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36757_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 36757_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52630_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52630_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69091_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 69091_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05451_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 05451_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:31.28 +40:55:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38296_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 38296_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71633_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 71633_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48026_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 48026_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 18:13:29.43 +45:31:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55144_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 55144_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50681_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 50681_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05999_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 05999_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:02.52 +41:00:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58381_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 58381_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:22:54.78 +46:12:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47749_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 47749_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52268_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52268_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48772_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 48772_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:22:35.84 +45:16:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50118_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 50118_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43113_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 43113_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50292_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 50292_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36268_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 36268_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48079_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 48079_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08284_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 08284_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:05.17 +41:13:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52059_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52059_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48111_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 48111_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82395_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 82395_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20125_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 20125_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:56:00.44 +42:52:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46072_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 46072_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:22:46.46 +45:00:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51902_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 51902_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36490_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 36490_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06640_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 06640_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:38.14 +41:03:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46319_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 46319_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:21:55.02 +45:01:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38466_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 38466_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51028_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 51028_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37152_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 37152_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28319_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 28319_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:18:09.13 +43:12:14.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37504_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 37504_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53234_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53234_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54411_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 54411_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11215_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 11215_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:20:07.95 +41:31:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36959_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 36959_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07755_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 07755_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:24.70 +41:12:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53096_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53096_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38096_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 38096_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56832_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 56832_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:24:30.14 +46:08:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55038_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 55038_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53689_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 53689_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21167_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 21167_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27352_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 27352_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:18:13.59 +43:06:51.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37842_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 37842_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42136_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 42136_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:26.95 +44:33:44.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08049_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 08049_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:45.60 +41:12:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07241_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 07241_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:31.48 +41:06:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91306_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 91306_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52845_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 52845_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25580_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 25580_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:19:43.62 +42:58:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56969_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 56969_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46497_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 46497_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:23:09.58 +45:03:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49882_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
Preparing report for the candidate 49882_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51687_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 51687_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:39:28.24 +46:00:25.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66693_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291
The candidate 66693_fd_Her-02-Q1b1x1_2026-07-10_02-49-51_20.00sec_-0.00C_LIGHTs_0291 did not pass the final checks
**** FOUND 17:49:04.25 +50:46:55.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 182s
Prepared the HTML report for the field Her-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:33:18.17 +40:47:31.4
17:58:09.21 +41:25:40.5
17:38:32.88 +42:51:12.8
18:28:21.34 +43:03:26.6
18:19:11.81 +44:18:30.4
18:21:13.57 +44:17:42.1
18:21:12.68 +44:21:18.0
18:38:28.17 +44:03:40.8
18:27:16.13 +44:16:55.4
18:19:51.90 +44:23:22.9
18:27:41.90 +44:17:59.4
18:28:43.22 +44:18:21.7
18:21:50.28 +44:25:51.4
18:27:14.80 +44:22:52.8
18:26:43.99 +44:23:50.3
18:37:48.48 +44:14:00.3
18:20:21.74 +44:31:16.3
18:21:10.95 +44:31:47.6
17:18:00.77 +44:37:31.4
17:23:32.74 +45:02:13.2
18:27:18.49 +45:18:37.1
17:20:37.84 +45:08:04.3
17:20:26.33 +45:09:41.7
17:20:31.35 +45:09:45.4
17:20:12.32 +45:09:27.3
17:20:12.33 +45:15:04.9
17:21:12.47 +45:21:17.9
17:20:55.47 +45:22:18.4
17:20:25.64 +45:22:45.2
17:20:29.49 +45:22:54.9
17:20:33.11 +45:24:45.0
17:23:05.87 +45:30:17.1
17:20:04.09 +45:31:53.1
18:27:30.46 +45:46:02.5
17:19:49.33 +45:32:24.9
17:20:25.86 +45:33:43.1
17:19:36.45 +45:33:55.9
17:21:11.95 +45:37:02.9
17:16:41.72 +45:30:54.3
17:20:20.33 +45:37:07.1
17:19:02.75 +45:36:16.4
17:21:46.41 +45:40:03.7
17:20:17.21 +45:39:01.5
17:21:48.44 +45:41:04.1
17:23:00.92 +45:43:25.7
17:18:40.59 +45:39:55.1
17:16:54.76 +45:41:31.3
17:23:06.90 +45:53:23.8
17:22:55.77 +45:53:23.3
17:22:00.57 +45:52:30.9
17:23:40.54 +45:56:30.0
17:23:36.84 +45:57:07.7
17:19:58.07 +45:57:15.3
17:20:27.43 +45:58:50.6
17:18:22.58 +46:08:09.8
17:51:45.09 +50:31:24.3
17:22:50.34 +46:46:50.3
17:54:20.42 +49:25:58.4
17:53:20.83 +48:33:31.7
17:54:41.41 +48:31:45.2
17:20:23.26 +47:12:21.4
########### Completed Her-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:28:21.34 +43:03:26.6
17:18:22.58 +46:08:09.8
17:20:23.26 +47:12:21.4
17:23:40.54 +45:56:30.0
18:19:11.81 +44:18:30.4
17:20:27.43 +45:58:50.6
18:19:51.90 +44:23:22.9
17:22:55.77 +45:53:23.3
17:19:36.45 +45:33:55.9
18:27:18.49 +45:18:37.1
17:58:09.21 +41:25:40.5
17:16:41.72 +45:30:54.3
17:23:00.92 +45:43:25.7
17:20:12.33 +45:15:04.9
18:21:13.57 +44:17:42.1
17:20:26.33 +45:09:41.7
17:53:20.83 +48:33:31.7
17:19:58.07 +45:57:15.3
17:20:17.21 +45:39:01.5
17:23:36.84 +45:57:07.7
18:33:18.17 +40:47:31.4
17:23:32.74 +45:02:13.2
17:19:49.33 +45:32:24.9
18:27:14.80 +44:22:52.8
17:19:02.75 +45:36:16.4
17:20:29.49 +45:22:54.9
18:27:16.13 +44:16:55.4
17:21:11.95 +45:37:02.9
17:51:45.09 +50:31:24.3
18:20:21.74 +44:31:16.3
17:22:50.34 +46:46:50.3
17:22:00.57 +45:52:30.9
17:20:33.11 +45:24:45.0
17:20:37.84 +45:08:04.3
17:20:25.86 +45:33:43.1
17:20:55.47 +45:22:18.4
17:18:00.77 +44:37:31.4
17:20:25.64 +45:22:45.2
18:21:12.68 +44:21:18.0
17:20:31.35 +45:09:45.4
18:27:30.46 +45:46:02.5
17:20:12.32 +45:09:27.3
17:54:20.42 +49:25:58.4
17:20:04.09 +45:31:53.1
18:38:28.17 +44:03:40.8
18:21:10.95 +44:31:47.6
17:23:05.87 +45:30:17.1
18:28:43.22 +44:18:21.7
18:21:50.28 +44:25:51.4
17:21:48.44 +45:41:04.1
17:16:54.76 +45:41:31.3
18:27:41.90 +44:17:59.4
17:21:46.41 +45:40:03.7
18:37:48.48 +44:14:00.3
17:23:06.90 +45:53:23.8
17:18:40.59 +45:39:55.1
17:38:32.88 +42:51:12.8
18:26:43.99 +44:23:50.3
17:54:41.41 +48:31:45.2
17:20:20.33 +45:37:07.1
17:21:12.47 +45:21:17.9
###################################################################################
18:28:21.34 +43:03:26.6 -- not an asteroid (will add it to exclusion list)
17:18:22.58 +46:08:09.8 -- not an asteroid (will add it to exclusion list)
17:20:23.26 +47:12:21.4 -- not an asteroid (will add it to exclusion list)
17:23:40.54 +45:56:30.0 -- not an asteroid (will add it to exclusion list)
18:19:11.81 +44:18:30.4 -- not an asteroid (will add it to exclusion list)
17:20:27.43 +45:58:50.6 -- not an asteroid (will add it to exclusion list)
18:19:51.90 +44:23:22.9 -- not an asteroid (will add it to exclusion list)
17:22:55.77 +45:53:23.3 -- not an asteroid (will add it to exclusion list)
17:19:36.45 +45:33:55.9 -- not an asteroid (will add it to exclusion list)
18:27:18.49 +45:18:37.1 -- not an asteroid (will add it to exclusion list)
17:58:09.21 +41:25:40.5 -- not an asteroid (will add it to exclusion list)
17:16:41.72 +45:30:54.3 -- not an asteroid (will add it to exclusion list)
17:23:00.92 +45:43:25.7 -- not an asteroid (will add it to exclusion list)
17:20:12.33 +45:15:04.9 -- not an asteroid (will add it to exclusion list)
18:21:13.57 +44:17:42.1 -- not an asteroid (will add it to exclusion list)
17:20:26.33 +45:09:41.7 -- not an asteroid (will add it to exclusion list)
17:53:20.83 +48:33:31.7 -- not an asteroid (will add it to exclusion list)
17:19:58.07 +45:57:15.3 -- not an asteroid (will add it to exclusion list)
17:20:17.21 +45:39:01.5 -- not an asteroid (will add it to exclusion list)
17:23:36.84 +45:57:07.7 -- not an asteroid (will add it to exclusion list)
18:33:18.17 +40:47:31.4 -- not an asteroid (will add it to exclusion list)
17:23:32.74 +45:02:13.2 -- not an asteroid (will add it to exclusion list)
17:19:49.33 +45:32:24.9 -- not an asteroid (will add it to exclusion list)
18:27:14.80 +44:22:52.8 -- not an asteroid (will add it to exclusion list)
17:19:02.75 +45:36:16.4 -- not an asteroid (will add it to exclusion list)
17:20:29.49 +45:22:54.9 -- not an asteroid (will add it to exclusion list)
18:27:16.13 +44:16:55.4 -- not an asteroid (will add it to exclusion list)
17:21:11.95 +45:37:02.9 -- not an asteroid (will add it to exclusion list)
17:51:45.09 +50:31:24.3 -- not an asteroid (will add it to exclusion list)
18:20:21.74 +44:31:16.3 -- not an asteroid (will add it to exclusion list)
17:22:50.34 +46:46:50.3 -- not an asteroid (will add it to exclusion list)
17:22:00.57 +45:52:30.9 -- not an asteroid (will add it to exclusion list)
17:20:33.11 +45:24:45.0 -- not an asteroid (will add it to exclusion list)
17:20:37.84 +45:08:04.3 -- not an asteroid (will add it to exclusion list)
17:20:25.86 +45:33:43.1 -- not an asteroid (will add it to exclusion list)
17:20:55.47 +45:22:18.4 -- not an asteroid (will add it to exclusion list)
17:18:00.77 +44:37:31.4 -- not an asteroid (will add it to exclusion list)
17:20:25.64 +45:22:45.2 -- not an asteroid (will add it to exclusion list)
18:21:12.68 +44:21:18.0 -- not an asteroid (will add it to exclusion list)
17:20:31.35 +45:09:45.4 -- not an asteroid (will add it to exclusion list)
18:27:30.46 +45:46:02.5 -- not an asteroid (will add it to exclusion list)
17:20:12.32 +45:09:27.3 -- not an asteroid (will add it to exclusion list)
17:54:20.42 +49:25:58.4 -- not an asteroid (will add it to exclusion list)
17:20:04.09 +45:31:53.1 -- not an asteroid (will add it to exclusion list)
18:38:28.17 +44:03:40.8 -- not an asteroid (will add it to exclusion list)
18:21:10.95 +44:31:47.6 -- not an asteroid (will add it to exclusion list)
17:23:05.87 +45:30:17.1 -- not an asteroid (will add it to exclusion list)
18:28:43.22 +44:18:21.7 -- not an asteroid (will add it to exclusion list)
18:21:50.28 +44:25:51.4 -- not an asteroid (will add it to exclusion list)
17:21:48.44 +45:41:04.1 -- not an asteroid (will add it to exclusion list)
17:16:54.76 +45:41:31.3 -- not an asteroid (will add it to exclusion list)
18:27:41.90 +44:17:59.4 -- not an asteroid (will add it to exclusion list)
17:21:46.41 +45:40:03.7 -- not an asteroid (will add it to exclusion list)
18:37:48.48 +44:14:00.3 -- not an asteroid (will add it to exclusion list)
17:23:06.90 +45:53:23.8 -- not an asteroid (will add it to exclusion list)
17:18:40.59 +45:39:55.1 -- not an asteroid (will add it to exclusion list)
17:38:32.88 +42:51:12.8 -- not an asteroid (will add it to exclusion list)
18:26:43.99 +44:23:50.3 -- not an asteroid (will add it to exclusion list)
17:54:41.41 +48:31:45.2 -- not an asteroid (will add it to exclusion list)
17:20:20.33 +45:37:07.1 -- not an asteroid (will add it to exclusion list)
17:21:12.47 +45:21:17.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:16:41.72 +45:30:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:54.76 +45:41:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:00.77 +44:37:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:22.58 +46:08:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:40.59 +45:39:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:02.75 +45:36:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:36.45 +45:33:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:49.33 +45:32:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:58.07 +45:57:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:04.09 +45:31:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:12.32 +45:09:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:12.33 +45:15:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:17.21 +45:39:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:20.33 +45:37:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:23.26 +47:12:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:25.64 +45:22:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:25.86 +45:33:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:26.33 +45:09:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:27.43 +45:58:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:29.49 +45:22:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:31.35 +45:09:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:33.11 +45:24:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:37.84 +45:08:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:55.47 +45:22:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:11.95 +45:37:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:12.47 +45:21:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:46.41 +45:40:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:48.44 +45:41:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:22:00.57 +45:52:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:22:50.34 +46:46:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:22:55.77 +45:53:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:00.92 +45:43:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:05.87 +45:30:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:06.90 +45:53:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:32.74 +45:02:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:36.84 +45:57:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:40.54 +45:56:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:38:32.88 +42:51:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:45.09 +50:31:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:53:20.83 +48:33:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:20.42 +49:25:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:41.41 +48:31:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:58:09.21 +41:25:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:11.81 +44:18:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:51.90 +44:23:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:21.74 +44:31:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:10.95 +44:31:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:12.68 +44:21:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:13.57 +44:17:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:50.28 +44:25:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:43.99 +44:23:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:14.80 +44:22:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:16.13 +44:16:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:18.49 +45:18:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:30.46 +45:46:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:41.90 +44:17:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:21.34 +43:03:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:28:43.22 +44:18:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:33:18.17 +40:47:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:48.48 +44:14:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:28.17 +44:03:40.8 -- 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)
17:16:41.72 +45:30:54.3 -- not a known variable star
17:16:54.76 +45:41:31.3 -- not a known variable star
17:18:00.77 +44:37:31.4 -- not a known variable star
17:18:22.58 +46:08:09.8 -- not a known variable star
17:18:40.59 +45:39:55.1 -- not a known variable star
17:19:02.75 +45:36:16.4 -- not a known variable star
17:19:36.45 +45:33:55.9 -- not a known variable star
17:19:49.33 +45:32:24.9 -- a known variable star
17:19:58.07 +45:57:15.3 -- not a known variable star
17:20:04.09 +45:31:53.1 -- not a known variable star
17:20:12.32 +45:09:27.3 -- not a known variable star
17:20:12.33 +45:15:04.9 -- not a known variable star
17:20:17.21 +45:39:01.5 -- not a known variable star
17:20:20.33 +45:37:07.1 -- not a known variable star
17:20:23.26 +47:12:21.4 -- not a known variable star
17:20:25.64 +45:22:45.2 -- not a known variable star
17:20:25.86 +45:33:43.1 -- not a known variable star
17:20:26.33 +45:09:41.7 -- not a known variable star
17:20:27.43 +45:58:50.6 -- not a known variable star
17:20:29.49 +45:22:54.9 -- a known variable star
17:20:31.35 +45:09:45.4 -- not a known variable star
17:20:33.11 +45:24:45.0 -- not a known variable star
17:20:37.84 +45:08:04.3 -- not a known variable star
17:20:55.47 +45:22:18.4 -- not a known variable star
17:21:11.95 +45:37:02.9 -- not a known variable star
17:21:12.47 +45:21:17.9 -- not a known variable star
17:21:46.41 +45:40:03.7 -- not a known variable star
17:21:48.44 +45:41:04.1 -- not a known variable star
17:22:00.57 +45:52:30.9 -- not a known variable star
17:22:50.34 +46:46:50.3 -- not a known variable star
17:22:55.77 +45:53:23.3 -- not a known variable star
17:23:00.92 +45:43:25.7 -- not a known variable star
17:23:05.87 +45:30:17.1 -- not a known variable star
17:23:06.90 +45:53:23.8 -- not a known variable star
17:23:32.74 +45:02:13.2 -- not a known variable star
17:23:36.84 +45:57:07.7 -- not a known variable star
17:23:40.54 +45:56:30.0 -- not a known variable star
17:38:32.88 +42:51:12.8 -- a known variable star
17:51:45.09 +50:31:24.3 -- not a known variable star
17:53:20.83 +48:33:31.7 -- not a known variable star
17:54:20.42 +49:25:58.4 -- a known variable star
17:54:41.41 +48:31:45.2 -- not a known variable star
17:58:09.21 +41:25:40.5 -- a known variable star
18:19:11.81 +44:18:30.4 -- not a known variable star
18:19:51.90 +44:23:22.9 -- not a known variable star
18:20:21.74 +44:31:16.3 -- not a known variable star
18:21:10.95 +44:31:47.6 -- not a known variable star
18:21:12.68 +44:21:18.0 -- not a known variable star
18:21:13.57 +44:17:42.1 -- not a known variable star
18:21:50.28 +44:25:51.4 -- not a known variable star
18:26:43.99 +44:23:50.3 -- not a known variable star
18:27:14.80 +44:22:52.8 -- not a known variable star
18:27:16.13 +44:16:55.4 -- not a known variable star
18:27:18.49 +45:18:37.1 -- not a known variable star
18:27:30.46 +45:46:02.5 -- not a known variable star
18:27:41.90 +44:17:59.4 -- not a known variable star
18:28:21.34 +43:03:26.6 -- a known variable star
18:28:43.22 +44:18:21.7 -- not a known variable star
18:33:18.17 +40:47:31.4 -- not a known variable star
18:37:48.48 +44:14:00.3 -- not a known variable star
18:38:28.17 +44:03:40.8 -- not a known variable star
Found 55 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
61 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 61 (excluding asteroids and hot pixels, 55 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)2461231.82585091 -observatory V36
07:32:20.55 +17:08:04.9 Mercury (5.1mag)
10:11:32.47 +12:41:38.9 Venus (-4.1mag)
04:24:05.90 +21:25:00.9 Mars (1.3mag)
08:16:39.20 +20:11:33.2 Jupiter (-1.8mag)
00:55:50.75 +03:20:28.3 Saturn (0.7mag)
04:07:13.75 +20:45:02.6 Uranus (5.8mag)
00:17:01.50 +00:20:41.3 Neptune (7.8mag)
20:30:55.08 -23:17:60.0 Pluto (14.4mag)
03:10:09.01 +22:11:54.0 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 03:12 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.82585091:
08:16:45.60 +20:11:11.2 Io (6.1mag)
08:16:41.62 +20:11:26.0 Europa (6.3mag)
08:16:56.20 +20:10:31.9 Ganymede (5.6mag)
08:17:07.28 +20:09:49.6 Callisto (6.8mag)
08:15:10.76 +19:55:42.2 Himalia (15.7mag)
08:16:37.91 +20:11:39.0 Thebe (16.6mag)
08:14:32.11 +20:00:12.1 Elara (17.6mag)
08:20:11.38 +20:05:44.1 Pasiphae (17.8mag)
08:21:37.14 +20:16:38.0 Carme (19.0mag)
00:55:40.55 +03:20:19.4 Titan (8.5mag)
00:55:45.51 +03:20:31.7 Rhea (9.8mag)
00:55:20.07 +03:19:37.4 Iapetus (11.2mag)
00:56:00.07 +03:20:47.1 Hyperion (14.5mag)
00:55:51.51 +03:17:42.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 03:12 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.82585091:
17:46:11.54 -33:00:09.1 JWST
16:11:17.95 +49:20:38.8 Chandra
01:29:23.96 +64:05:06.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 03:12 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.82585091 -observatory V36
02:36:13.97 +14:25:30.6 17.9mag P/1996 R2 (Lagerkvist)
18:17:57.59 -34:21:42.9 13.7mag P/2010 H2 (Vales)
06:25:38.92 -68:08:21.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:47.83 +32:26:47.5 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.41 +16:02:55.0 18.0mag C/2021 G2 (ATLAS)
01:47:39.48 +08:10:07.7 15.4mag P/2021 N1 (ZTF)
22:59:32.81 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:22.19 +26:55:35.4 16.7mag C/2022 N2 (PANSTARRS)
09:55:29.55 +29:46:55.4 16.8mag C/2022 QE78 (ATLAS)
09:09:43.11 +04:59:55.3 17.8mag C/2022 R6 (PANSTARRS)
18:07:14.04 +21:17:41.4 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.39 -11:23:13.9 17.7mag P/2023 B1 (PANSTARRS)
21:49:15.96 +67:37:17.1 17.8mag C/2023 H5 (Lemmon)
16:30:56.23 -10:04:31.9 13.9mag C/2023 R1 (PANSTARRS)
08:00:36.32 +65:42:25.4 17.9mag C/2024 A1 (ATLAS)
07:32:46.81 +30:00:07.2 14.6mag C/2024 E1 (Wierzchos)
15:16:20.33 +15:19:39.6 17.5mag C/2024 G6 (ATLAS)
19:41:20.57 +39:23:16.6 13.8mag C/2024 J3 (ATLAS)
21:47:36.57 +45:59:57.5 17.8mag C/2024 R4 (PANSTARRS)
04:49:36.88 -13:47:49.5 15.7mag C/2024 T5 (ATLAS)
06:34:33.08 +29:04:27.0 18.0mag C/2025 J1 (Borisov)
07:14:19.22 -12:53:14.6 16.5mag C/2025 R3 (PANSTARRS)
09:56:03.69 +22:26:16.7 17.6mag C/2025 V2 (Rankin)
12:44:36.50 +03:56:20.1 17.1mag C/2025 Y1 (ATLAS)
16:52:01.73 +79:07:11.3 17.4mag C/2026 A2 (Bok)
02:46:14.86 +45:14:19.1 16.7mag C/2026 B2 (Sun-Gao)
11:25:29.67 +04:32:22.0 16.9mag A/2026 E1
21:18:59.88 -15:04:02.0 7.3mag 10P/Tempel
11:13:26.56 -01:53:09.9 16.1mag 29P/Schwassmann-Wachmann
04:00:08.05 +29:33:01.0 17.8mag 47P/Ashbrook-Jackson
10:08:01.27 +14:01:11.3 17.0mag 63P/Wild
00:48:21.05 -05:05:36.5 15.5mag 65P/Gunn
08:26:52.22 +34:13:12.2 17.9mag 76P/West-Kohoutek-Ikemura
04:27:20.05 +20:10:38.4 13.7mag 78P/Gehrels
02:22:17.47 +10:36:20.9 16.2mag 88P/Howell
06:35:27.08 +30:32:10.5 15.7mag 93P/Lovas
04:20:54.81 +31:07:18.4 16.9mag 114P/Wiseman-Skiff
08:08:37.77 +30:42:23.0 15.3mag 123P/West-Hartley
10:48:04.90 +01:11:51.6 16.8mag 124P/Mrkos
04:51:41.13 +20:48:43.8 16.2mag 128P/Shoemaker-Holt
05:36:12.32 +19:42:51.1 17.8mag 131P/Mueller
00:01:32.29 +02:56:03.0 17.9mag 139P/Vaisala-Oterma
07:13:27.79 +17:01:34.9 15.5mag 141P-D/Machholz
03:16:50.25 -21:06:29.2 15.5mag 161P/Hartley-IRAS
05:32:58.07 +33:56:34.0 15.3mag 162P/SidingSpring
19:04:32.47 +15:03:59.8 14.7mag 169P/NEAT
01:40:58.02 +07:35:44.2 17.7mag 220P/McNaught
16:35:58.39 -08:23:03.8 17.0mag 235P/LINEAR
08:45:13.76 +33:18:06.7 17.9mag 240P/NEAT
20:42:11.25 -49:33:53.0 17.8mag 259P/Garradd
01:59:13.95 +12:04:56.5 15.7mag 260P/McNaught
05:37:08.73 +36:50:26.5 17.4mag 295P/LINEAR
15:06:36.89 +06:03:33.3 17.6mag 391P/Kowalski
08:34:34.78 +19:40:40.2 17.9mag 450P/LONEOS
07:51:43.48 +39:13:06.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 03:12 comets.txt
############################################################
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 10 03:12 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
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
-rw-r--r-- 1 apache apache 189K Jul 10 03:12 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
20:52:11.463 -28:17:09.07 AT 2026spm 2026-07-07.32 21.7705
-rw-r--r-- 1 apache apache 30K Jul 10 03:12 tns_transients_list.txt
