This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.93 16:39:50.02 +16:49:09.6
34.38821 36.49078 galactic Her Second-epoch detections are separated by 3.3" and 8.9 pix
The object was found in VSX 5" CSS_J163950.0+164903
Type: RRC
# Max. Min./Amp. JD0 Period
13.520 g Y 0.562 g 2458605.90490 0.350407000000
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:50.02 +16:49:09.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:50.02 +16:49:09.6: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 50.02 +16 49 09.6 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
CSS_J163950.0+164903,2461237.8208,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J163950.0+164903 20260716.3208 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.57 17:18:25.73 +13:09:18.2
34.67717 26.48129 galactic Her Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541512025247605760 | 17:18:25.62 +13:09:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:25.73 +13:09:18.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:25.73 +13:09:18.2: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 25.73 +13 09 18.2 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541512025247605760,2461237.8208,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541512025247605760 20260716.3208 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.43 16:37:59.87 +16:34:10.2
33.89609 36.80666 galactic Her Second-epoch detections are separated by 1.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:37:59.87 +16:34:10.2 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:37:59.87 +16:34:10.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:37:59.87 +16:34:10.2: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 37 59.87 +16 34 10.2 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 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 16.3208 2461237.8208 12.23 16:45:40.32 +16:50:39.7
35.05319 35.20165 galactic Her Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:45:40.32 +16:50:39.7 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.033 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:40.32 +16:50:39.7: 13.17 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:40.32 +16:50:39.7: 13.18 +/- 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 16.3208* 16 45 40.32 +16 50 39.7 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.00 17:20:04.58 +13:09:14.1
34.85802 26.11445 galactic Her Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541502614976653056 | 17:20:04.54 +13:09:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.431+/-0.027 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:04.58 +13:09:14.1: 11.91 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:04.58 +13:09:14.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 20 04.58 +13 09 14.1 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541502614976653056,2461237.8208,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541502614976653056 20260716.3208 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.19 16:42:51.40 +10:54:42.5
28.13594 33.45553 galactic Her Second-epoch detections are separated by 2.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:42:51.40 +10:54:42.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.566+/-0.032 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:51.40 +10:54:42.5: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:51.40 +10:54:42.5: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 51.40 +10 54 42.5 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.05 16:38:42.59 +16:18:19.2
33.66989 36.54971 galactic Her Second-epoch detections are separated by 0.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4463019234467784192 | 16:38:42.60 +16:18:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.819+/-0.028 (M)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:42.59 +16:18:19.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:42.59 +16:18:19.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 42.59 +16 18 19.2 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4463019234467784192,2461237.8208,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4463019234467784192 20260716.3208 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.24 16:42:36.07 +10:36:58.2
27.78388 33.38485 galactic Her Second-epoch detections are separated by 2.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:42:36.07 +10:36:58.2 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.044 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:36.07 +10:36:58.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:36.07 +10:36:58.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 36.07 +10 36 58.2 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.11 16:39:06.52 +16:12:26.3
33.60153 36.42421 galactic Her Second-epoch detections are separated by 1.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:06.52 +16:12:26.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.695+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:06.52 +16:12:26.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:06.52 +16:12:26.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 06.52 +16 12 26.3 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,2461237.8208,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.20 16:42:29.99 +10:45:08.8
27.91832 33.46610 galactic Her Second-epoch detections are separated by 1.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:42:29.99 +10:45:08.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.344+/-0.035 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:29.99 +10:45:08.8: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:29.99 +10:45:08.8: 13.31 +/- 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 16.3208* 16 42 29.99 +10 45 08.8 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.13 17:20:56.49 +13:23:52.4
35.20139 26.02117 galactic Oph Second-epoch detections are separated by 1.0" and 8.2 pix
The object was found in VSX 9" Gaia DR3 4543009594443761536
Type: ROT
# Max. Min./Amp. JD0 Period
17.240 G 17.290 G K
ATTENTION: measured mag 11.13 is 6.1 mag brighter than the VSX record maximum brightness 17.24 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:56.49 +13:23:52.4: 12.13 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:56.49 +13:23:52.4: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4543009594443761536,2461237.8208,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4543009594443761536 20260716.3208 11.13CV 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 16.3208 2461237.8208 11.18 16:39:56.22 +13:15:03.4
30.34582 35.08230 galactic Her Second-epoch detections are separated by 0.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4461146761867570560 | 16:39:56.21 +13:15:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:56.22 +13:15:03.4: 12.11 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:56.22 +13:15:03.4: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 56.22 +13 15 03.4 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4461146761867570560,2461237.8208,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4461146761867570560 20260716.3208 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.68 17:21:22.48 +13:18:59.4
35.16619 25.89185 galactic Oph Second-epoch detections are separated by 2.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4542257154831155200 | 17:21:22.56 +13:18:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.820+/-0.025 (M)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:22.48 +13:18:59.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:22.48 +13:18:59.4: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4542257154831155200,2461237.8208,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4542257154831155200 20260716.3208 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.59 17:19:30.60 +13:28:28.9
35.12257 26.37054 galactic Her Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541526907311716352 | 17:19:30.51 +13:28:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.548+/-0.028 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:30.60 +13:28:28.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:30.60 +13:28:28.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 30.60 +13 28 28.9 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541526907311716352,2461237.8208,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541526907311716352 20260716.3208 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.76 17:11:11.47 +15:48:00.8
36.63911 29.13746 galactic Her Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4546752542480919296 | 17:11:11.47 +15:48:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:11:11.47 +15:48:00.8: 12.62 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:11:11.47 +15:48:00.8: 12.63 +/- 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 16.3208* 17 11 11.47 +15 48 00.8 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4546752542480919296,2461237.8208,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4546752542480919296 20260716.3208 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.56 16:42:12.40 +10:55:35.0
28.06957 33.60590 galactic Her Second-epoch detections are separated by 0.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4446983956887145344 | 16:42:12.41 +10:55:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.029 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:12.40 +10:55:35.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:12.40 +10:55:35.0: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 12.40 +10 55 35.0 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4446983956887145344,2461237.8208,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4446983956887145344 20260716.3208 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.12 17:18:38.07 +13:36:11.6
35.15787 26.61712 galactic Her Second-epoch detections are separated by 0.3" and 8.3 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 J259.6548+13.6010 | 17:18:38.08 +13:36:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.028 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:38.07 +13:36:11.6: 12.07 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:38.07 +13:36:11.6: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 38.07 +13 36 11.6 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.6548+13.6010,2461237.8208,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.6548+13.6010 20260716.3208 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.14 17:19:22.05 +13:39:07.3
35.28810 26.47384 galactic Her Second-epoch detections are separated by 1.6" and 8.1 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 | 17:19:22.05 +13:39:07.3 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.028 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:22.05 +13:39:07.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:22.05 +13:39:07.3: 13.24 +/- 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 16.3208* 17 19 22.05 +13 39 07.3 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,2461237.8208,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.99 17:21:11.60 +12:34:19.0
34.39159 25.62796 galactic Oph Second-epoch detections are separated by 3.3" and 9.0 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 4540667913852319488 | 17:21:10.62 +12:34:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.321+/-0.038 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:11.60 +12:34:19.0: 12.99 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:11.60 +12:34:19.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4540667913852319488,2461237.8208,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4540667913852319488 20260716.3208 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.19 16:40:28.09 +16:11:09.5
33.72915 36.11373 galactic Her Second-epoch detections are separated by 0.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:40:28.09 +16:11:09.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.560+/-0.031 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:28.09 +16:11:09.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:28.09 +16:11:09.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 40 28.09 +16 11 09.5 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.20 16:40:42.36 +16:14:35.6
33.82135 36.08233 galactic Her Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:40:42.36 +16:14:35.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.277+/-0.030 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:42.36 +16:14:35.6: 13.25 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:42.36 +16:14:35.6: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 40 42.36 +16 14 35.6 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.91 16:39:33.44 +13:12:23.6
30.25025 35.14861 galactic Her Second-epoch detections are separated by 1.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:33.44 +13:12:23.6 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.028 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:33.44 +13:12:23.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:33.44 +13:12:23.6: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 33.44 +13 12 23.6 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.77 16:42:33.59 +10:52:39.2
28.06133 33.50663 galactic Her Second-epoch detections are separated by 0.8" and 8.7 pix
The object was found in VSX 0" Gaia DR3 4446980417834066688
Type: ROT
# Max. Min./Amp. JD0 Period
12.760 G 12.800 G G
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:33.59 +10:52:39.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:33.59 +10:52:39.2: 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!
TCP 2026 07 16.3208* 16 42 33.59 +10 52 39.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4446980417834066688,2461237.8208,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4446980417834066688 20260716.3208 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.29 16:50:34.02 +14:20:16.3
32.79869 33.15375 galactic Her Second-epoch detections are separated by 2.1" and 8.1 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 | 16:50:34.02 +14:20:16.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.383+/-0.026 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:50:34.02 +14:20:16.3: 13.21 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:50:34.02 +14:20:16.3: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 50 34.02 +14 20 16.3 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.23 16:45:52.79 +16:31:03.0
34.70473 35.03410 galactic Her Second-epoch detections are separated by 2.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:45:52.79 +16:31:03.0 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.638+/-0.033 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:52.79 +16:31:03.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:52.79 +16:31:03.0: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 45 52.79 +16 31 03.0 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.16 16:38:50.38 +16:39:58.8
34.10165 36.65532 galactic Her Second-epoch detections are separated by 3.2" and 8.0 pix
The object was found in VSX 1" Gaia DR3 4466037600044019712
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:50.38 +16:39:58.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:50.38 +16:39:58.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 50.38 +16 39 58.8 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4466037600044019712,2461237.8208,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4466037600044019712 20260716.3208 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.06 16:50:48.91 +15:20:44.6
33.93721 33.49192 galactic Her Second-epoch detections are separated by 1.6" and 8.1 pix
The object was found in VSX 1" ZTF J165048.86+152044.3
Type: HADS
# Max. Min./Amp. JD0 Period
13.206 g Y 0.202 g 2458362.75500 0.052177700000
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:50:48.91 +15:20:44.6: 13.16 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:50:48.91 +15:20:44.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 50 48.91 +15 20 44.6 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
ZTF J165048.86+152044.3,2461237.8208,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J165048.86+152044.3 20260716.3208 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 16.3208 2461237.8208 12.22 16:40:13.21 +16:50:21.2
34.45361 36.41215 galactic Her Second-epoch detections are separated by 2.3" and 8.1 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 | 16:40:13.21 +16:50:21.2 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.033 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:13.21 +16:50:21.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:13.21 +16:50:21.2: 13.17 +/- 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 16.3208* 16 40 13.21 +16 50 21.2 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.23 16:45:44.83 +16:47:32.6
35.00224 35.16572 galactic Her Second-epoch detections are separated by 2.0" and 8.6 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 J251.4391+16.7917 | 16:45:44.83 +16:47:32.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.317+/-0.036 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:44.83 +16:47:32.6: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:44.83 +16:47:32.6: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 45 44.83 +16 47 32.6 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
ATO J251.4391+16.7917,2461237.8208,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J251.4391+16.7917 20260716.3208 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.98 16:43:00.03 +10:41:08.3
27.90961 33.32634 galactic Her Second-epoch detections are separated by 0.7" and 8.5 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 | ASAS J164302+1041.2 | 16:43:02.47 +10:41:07.0 (Gaia DR3) | MISC (local) | 2.509318000000 (local) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.394+/-0.032 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:43:00.03 +10:41:08.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:43:00.03 +10:41:08.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 43 00.03 +10 41 08.3 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164302+1041.2,2461237.8208,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J164302+1041.2 20260716.3208 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 10.96 16:42:40.72 +10:48:45.9
28.00622 33.45243 galactic Her Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4446979180883466112 | 16:42:40.71 +10:48:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.033 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:40.72 +10:48:45.9: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:40.72 +10:48:45.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 40.72 +10 48 45.9 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4446979180883466112,2461237.8208,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4446979180883466112 20260716.3208 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.62 17:19:04.30 +12:53:14.9
34.47575 26.22922 galactic Her Second-epoch detections are separated by 1.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4540718487089343104 | 17:19:04.28 +12:53:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.901+/-0.028 (M)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:04.30 +12:53:14.9: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:04.30 +12:53:14.9: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 04.30 +12 53 14.9 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4540718487089343104,2461237.8208,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4540718487089343104 20260716.3208 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.59 17:19:02.99 +12:46:48.5
34.36416 26.19016 galactic Her Second-epoch detections are separated by 2.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J259.7639+12.7910 | 17:19:02.97 +12:46:48.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.464+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:02.99 +12:46:48.5: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:02.99 +12:46:48.5: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 02.99 +12 46 48.5 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.7639+12.7910,2461237.8208,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.7639+12.7910 20260716.3208 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.63 17:18:36.81 +13:15:22.9
34.80099 26.48139 galactic Her Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541514464788497280 | 17:18:36.79 +13:15:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:36.81 +13:15:22.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:36.81 +13:15:22.9: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 36.81 +13 15 22.9 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541514464788497280,2461237.8208,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541514464788497280 20260716.3208 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.38 16:39:50.10 +16:51:39.5
34.43651 36.50584 galactic Her Second-epoch detections are separated by 2.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:50.10 +16:51:39.5 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:50.10 +16:51:39.5: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:50.10 +16:51:39.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 50.10 +16 51 39.5 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.80 16:38:46.34 +16:19:35.3
33.70128 36.54372 galactic Her Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:38:46.34 +16:19:35.3 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.656+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:46.34 +16:19:35.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:46.34 +16:19:35.3: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 46.34 +16 19 35.3 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.15 16:39:37.21 +16:27:20.6
33.94486 36.40340 galactic Her Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:37.21 +16:27:20.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.621+/-0.029 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:37.21 +16:27:20.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:37.21 +16:27:20.6: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 37.21 +16 27 20.6 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 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 16.3208 2461237.8208 11.81 16:40:07.24 +16:28:21.5
34.01990 36.29837 galactic Her Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:40:07.24 +16:28:21.5 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.034 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:07.24 +16:28:21.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:07.24 +16:28:21.5: 12.86 +/- 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 16.3208* 16 40 07.24 +16 28 21.5 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.32 16:36:20.05 +12:05:34.2
28.60981 35.40366 galactic Her Second-epoch detections are separated by 2.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:36:20.05 +12:05:34.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.696+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:36:20.05 +12:05:34.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:36:20.05 +12:05:34.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 36 20.05 +12 05 34.2 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.31 17:16:28.86 +14:02:00.0
35.36412 27.26866 galactic Her Second-epoch detections are separated by 1.9" and 8.1 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 | 17:16:28.86 +14:02:00.0 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.035 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:16:28.86 +14:02:00.0: 13.82 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:16:28.86 +14:02:00.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 16 28.86 +14 02 00.0 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.46 16:39:12.90 +16:42:31.1
34.19208 36.58749 galactic Her Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4466038940073812864 | 16:39:13.00 +16:42:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.457+/-0.033 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:12.90 +16:42:31.1: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:12.90 +16:42:31.1: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 12.90 +16 42 31.1 11.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4466038940073812864,2461237.8208,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4466038940073812864 20260716.3208 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.63 17:18:50.61 +12:33:04.9
34.10869 26.14219 galactic Oph Second-epoch detections are separated by 2.2" and 8.1 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 J259.7110+12.5551 | 17:18:50.61 +12:33:05.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.528+/-0.027 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:50.61 +12:33:04.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:50.61 +12:33:04.9: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.7110+12.5551,2461237.8208,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.7110+12.5551 20260716.3208 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.17 16:39:34.06 +16:36:12.0
34.10934 36.47001 galactic Her Second-epoch detections are separated by 1.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:34.06 +16:36:12.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.461+/-0.029 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:34.06 +16:36:12.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:34.06 +16:36:12.0: 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 16.3208* 16 39 34.06 +16 36 12.0 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 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 16.3208 2461237.8208 12.17 16:42:17.27 +10:47:19.6
27.93075 33.52874 galactic Her Second-epoch detections are separated by 1.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:42:17.27 +10:47:19.6 (user input) | T | P | (position from user input) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:17.27 +10:47:19.6: 13.17 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:17.27 +10:47:19.6: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 17.27 +10 47 19.6 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 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 16.3208 2461237.8208 12.23 16:41:07.26 +10:04:55.6
27.01793 33.48040 galactic Her Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:41:07.26 +10:04:55.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.406+/-0.029 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:41:07.26 +10:04:55.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:41:07.26 +10:04:55.6: 13.12 +/- 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!
TCP 2026 07 16.3208* 16 41 07.26 +10 04 55.6 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.18 16:49:30.77 +15:20:44.0
33.79170 33.78158 galactic Her Second-epoch detections are separated by 1.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:49:30.77 +15:20:44.0 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:49:30.77 +15:20:44.0: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:49:30.77 +15:20:44.0: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 49 30.77 +15 20 44.0 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.99 17:19:46.78 +13:27:15.2
35.13128 26.30230 galactic Her Second-epoch detections are separated by 0.7" and 8.4 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 | 17:19:46.78 +13:27:15.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.339+/-0.031 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:46.78 +13:27:15.2: 13.12 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:46.78 +13:27:15.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 46.78 +13 27 15.2 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,2461237.8208,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.82 16:39:07.37 +16:27:06.2
33.88495 36.51255 galactic Her Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:07.37 +16:27:06.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.703+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:07.37 +16:27:06.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:07.37 +16:27:06.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 07.37 +16 27 06.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.85 17:18:59.32 +13:35:43.6
35.18875 26.53524 galactic Her Second-epoch detections are separated by 1.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J259.7464+13.5993 | 17:18:59.32 +13:35:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.522+/-0.029 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:59.32 +13:35:43.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:59.32 +13:35:43.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 59.32 +13 35 43.6 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.7464+13.5993,2461237.8208,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.7464+13.5993 20260716.3208 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.97 17:21:27.74 +13:16:27.0
35.13282 25.85517 galactic Oph Second-epoch detections are separated by 1.8" and 8.7 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 J260.3670+13.2703 | 17:21:27.74 +13:16:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.712+/-0.025 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:27.74 +13:16:27.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:27.74 +13:16:27.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J260.3670+13.2703,2461237.8208,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.3670+13.2703 20260716.3208 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.13 16:46:08.79 +16:31:01.9
34.73349 34.97468 galactic Her Second-epoch detections are separated by 1.3" and 8.4 pix
The object was found in VSX 1" Gaia DR3 4558891975485708160
Type: VAR
# Max. Min./Amp. JD0 Period
12.890 G 12.950 G 0.155413200000 K
The object was not found in astcheck.
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:46:08.79 +16:31:01.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:46:08.79 +16:31:01.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 46 08.79 +16 31 01.9 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4558891975485708160,2461237.8208,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4558891975485708160 20260716.3208 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 16.3208 2461237.8208 12.45 16:38:45.32 +16:50:00.0
34.28587 36.73580 galactic Her Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:38:45.32 +16:50:00.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.361+/-0.033 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:45.32 +16:50:00.0: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:45.32 +16:50:00.0: 13.72 +/- 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!
TCP 2026 07 16.3208* 16 38 45.32 +16 50 00.0 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.80 16:39:45.03 +16:40:45.2
34.21717 36.45748 galactic Her Second-epoch detections are separated by 0.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:45.03 +16:40:45.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.281+/-0.031 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:45.03 +16:40:45.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:45.03 +16:40:45.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 45.03 +16 40 45.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.63 17:18:23.44 +13:06:25.0
34.62385 26.47020 galactic Her Second-epoch detections are separated by 0.9" and 8.6 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 J259.5976+13.1069 | 17:18:23.44 +13:06:25.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M2 (LAMOST DR5) J-Ks=1.109+/-0.029 (M)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:23.44 +13:06:25.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:23.44 +13:06:25.0: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 23.44 +13 06 25.0 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.5976+13.1069,2461237.8208,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.5976+13.1069 20260716.3208 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.39 16:38:19.84 +16:41:32.4
34.07546 36.77818 galactic Her Second-epoch detections are separated by 1.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:38:19.84 +16:41:32.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.355+/-0.035 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:19.84 +16:41:32.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:19.84 +16:41:32.4: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 19.84 +16 41 32.4 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.95 16:39:14.13 +16:25:39.0
33.86953 36.47844 galactic Her Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:14.13 +16:25:39.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:14.13 +16:25:39.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:14.13 +16:25:39.0: 13.11 +/- 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 16.3208* 16 39 14.13 +16 25 39.0 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.32 17:18:31.11 +13:08:45.3
34.67777 26.45763 galactic Her Second-epoch detections are separated by 1.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541511200613885312 | 17:18:31.11 +13:08:45.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.711+/-0.028 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:31.11 +13:08:45.3: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:31.11 +13:08:45.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 31.11 +13 08 45.3 11.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541511200613885312,2461237.8208,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541511200613885312 20260716.3208 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.46 17:18:45.37 +13:31:48.5
35.09645 26.56056 galactic Her Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541574937928018048 | 17:18:45.32 +13:31:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.028 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:45.37 +13:31:48.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:45.37 +13:31:48.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 18 45.37 +13 31 48.5 11.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541574937928018048,2461237.8208,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541574937928018048 20260716.3208 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.47 16:36:00.88 +12:03:53.9
28.53851 35.46284 galactic Her Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4459361537241260160 | 16:36:00.81 +12:03:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.031+/-0.032 (M)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:36:00.88 +12:03:53.9: 12.35 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:36:00.88 +12:03:53.9: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 36 00.88 +12 03 53.9 11.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4459361537241260160,2461237.8208,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4459361537241260160 20260716.3208 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.79 16:35:13.71 +12:14:08.8
28.63006 35.70890 galactic Her Second-epoch detections are separated by 1.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:35:13.71 +12:14:08.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.382+/-0.028 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:35:13.71 +12:14:08.8: 12.77 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:35:13.71 +12:14:08.8: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 35 13.71 +12 14 08.8 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.75 17:19:16.63 +13:40:49.6
35.30727 26.50538 galactic Her Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4543078386937847296 | 17:19:16.57 +13:40:49.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.344+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:16.63 +13:40:49.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:16.63 +13:40:49.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 16.63 +13 40 49.6 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4543078386937847296,2461237.8208,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4543078386937847296 20260716.3208 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.12 16:47:38.40 +17:22:31.9
35.86780 34.95905 galactic Her Second-epoch detections are separated by 2.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:47:38.40 +17:22:31.9 (user input) | T | P | (position from user input) J-Ks=0.660+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:47:38.40 +17:22:31.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:47:38.40 +17:22:31.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 47 38.40 +17 22 31.9 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.44 16:42:43.44 +10:45:24.2
27.95137 33.41826 galactic Her Second-epoch detections are separated by 0.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4446961176380547200 | 16:42:43.46 +10:45:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.035 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:43.44 +10:45:24.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:43.44 +10:45:24.2: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 43.44 +10 45 24.2 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4446961176380547200,2461237.8208,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4446961176380547200 20260716.3208 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.36 16:35:11.99 +12:10:56.1
28.56660 35.69283 galactic Her Second-epoch detections are separated by 1.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J248.7999+12.1826 | 16:35:11.99 +12:10:56.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.637+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:35:11.99 +12:10:56.1: 13.36 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:35:11.99 +12:10:56.1: 13.43 +/- 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 16.3208* 16 35 11.99 +12 10 56.1 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
ATO J248.7999+12.1826,2461237.8208,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J248.7999+12.1826 20260716.3208 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.08 16:38:36.87 +16:55:29.3
34.37656 36.80080 galactic Her Second-epoch detections are separated by 1.2" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:38:36.87 +16:55:29.3 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.613+/-0.027 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:36.87 +16:55:29.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:36.87 +16:55:29.3: 13.07 +/- 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 16.3208* 16 38 36.87 +16 55 29.3 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,2461237.8208,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.22 16:39:17.28 +16:48:26.7
34.31445 36.60776 galactic Her Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:17.28 +16:48:26.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.503+/-0.033 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:17.28 +16:48:26.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:17.28 +16:48:26.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 17.28 +16 48 26.7 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.48 16:39:33.56 +16:09:37.9
33.59821 36.30636 galactic Her Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:33.56 +16:09:37.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:33.56 +16:09:37.9: 13.56 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:33.56 +16:09:37.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 33.56 +16 09 37.9 12.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.29 16:38:04.38 +16:27:07.3
33.76834 36.74622 galactic Her Second-epoch detections are separated by 0.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:38:04.38 +16:27:07.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.406+/-0.034 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:04.38 +16:27:07.3: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:04.38 +16:27:07.3: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 04.38 +16 27 07.3 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.39 16:41:11.19 +11:57:49.1
29.07369 34.27255 galactic Her Second-epoch detections are separated by 0.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:41:11.19 +11:57:49.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.323+/-0.033 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:41:11.19 +11:57:49.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:41:11.19 +11:57:49.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 41 11.19 +11 57 49.1 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.38 16:39:09.78 +16:22:29.2
33.80063 36.47488 galactic Her Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:39:09.78 +16:22:29.2 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.298+/-0.034 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:09.78 +16:22:29.2: 13.61 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:09.78 +16:22:29.2: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 09.78 +16 22 29.2 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.46 16:40:21.21 +16:04:17.7
33.58515 36.09617 galactic Her Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:40:21.21 +16:04:17.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.550+/-0.035 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:21.21 +16:04:17.7: 13.56 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:21.21 +16:04:17.7: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 40 21.21 +16 04 17.7 12.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.88 17:01:39.61 +13:24:17.1
33.05752 30.31279 galactic Her Second-epoch detections are separated by 1.6" and 8.6 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 | 17:01:39.61 +13:24:17.1 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.028 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:01:39.61 +13:24:17.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:01:39.61 +13:24:17.1: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 01 39.61 +13 24 17.1 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.34 17:19:15.09 +13:09:35.6
34.77304 26.30031 galactic Her Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541500308576292608 | 17:19:15.01 +13:09:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.028 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:15.09 +13:09:35.6: 12.28 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:15.09 +13:09:35.6: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 15.09 +13 09 35.6 11.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541500308576292608,2461237.8208,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541500308576292608 20260716.3208 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.22 17:19:19.61 +13:24:07.7
35.02839 26.38189 galactic Her Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4541523192162039168 | 17:19:19.61 +13:24:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.365+/-0.027 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:19.61 +13:24:07.7: 12.25 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:19.61 +13:24:07.7: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 19.61 +13 24 07.7 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4541523192162039168,2461237.8208,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4541523192162039168 20260716.3208 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.81 16:42:11.03 +10:55:02.4
28.05686 33.60707 galactic Her Second-epoch detections are separated by 0.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4446983956887145344 | 16:42:12.41 +10:55:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.030 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:11.03 +10:55:02.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:11.03 +10:55:02.4: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 42 11.03 +10 55 02.4 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4446983956887145344,2461237.8208,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4446983956887145344 20260716.3208 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.22 17:20:18.05 +13:26:29.9
35.17565 26.18133 galactic Her Second-epoch detections are separated by 2.4" and 8.1 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 | 17:20:18.05 +13:26:29.9 (user input) | T | P | (position from user input) J-Ks=0.718+/-0.030 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:18.05 +13:26:29.9: 13.55 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:18.05 +13:26:29.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 20 18.05 +13 26 29.9 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
target,2461237.8208,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.11 17:18:31.88 +13:31:10.9
35.06108 26.60633 galactic Her Second-epoch detections are separated by 0.9" and 8.5 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 | 17:18:31.88 +13:31:10.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:31.88 +13:31:10.9: 13.29 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:31.88 +13:31:10.9: 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 16.3208* 17 18 31.88 +13 31 10.9 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.26 16:39:28.61 +13:11:58.0
30.23254 35.16360 galactic Her Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4461151988846658048 | 16:39:28.61 +13:11:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.687+/-0.026 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:28.61 +13:11:58.0: 12.24 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:28.61 +13:11:58.0: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 39 28.61 +13 11 58.0 11.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4461151988846658048,2461237.8208,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4461151988846658048 20260716.3208 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.18 16:38:31.03 +16:32:43.5
33.92591 36.68218 galactic Her Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J249.6292+16.5455 | 16:38:31.03 +16:32:43.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.626+/-0.027 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:31.03 +16:32:43.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:31.03 +16:32:43.5: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 16 38 31.03 +16 32 43.5 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J249.6292+16.5455,2461237.8208,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J249.6292+16.5455 20260716.3208 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 12.33 16:40:00.39 +13:16:02.6
30.37259 35.07355 galactic Her Second-epoch detections are separated by 1.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:40:00.39 +13:16:02.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.186+/-0.035 (F)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:00.39 +13:16:02.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:00.39 +13:16:02.6: 13.60 +/- 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!
TCP 2026 07 16.3208* 16 40 00.39 +13 16 02.6 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8208,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3208 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.66 17:19:59.23 +13:29:53.1
35.19879 26.27391 galactic Her Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4543025399923503232 | 17:19:59.18 +13:29:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.431+/-0.026 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:59.23 +13:29:53.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:59.23 +13:29:53.1: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 19 59.23 +13 29 53.1 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4543025399923503232,2461237.8208,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4543025399923503232 20260716.3208 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.57 17:20:22.44 +13:29:18.3
35.23134 26.18400 galactic Her Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4543014198648795648 | 17:20:22.41 +13:29:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.359+/-0.028 (G)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:22.44 +13:29:18.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:22.44 +13:29:18.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 20 22.44 +13 29 18.3 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4543014198648795648,2461237.8208,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4543014198648795648 20260716.3208 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3208 2461237.8208 11.12 17:20:41.04 +13:28:10.8
35.24621 26.10749 galactic Her Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4543013545813767168 | 17:20:41.04 +13:28:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.783+/-0.031 (K)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:41.04 +13:28:10.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:41.04 +13:28:10.8: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3208* 17 20 41.04 +13 28 10.8 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4543013545813767168,2461237.8208,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4543013545813767168 20260716.3208 11.12CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461209.78629625 18.06.2026 06:52:05.996 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
First image: 2461209.78629625 18.06.2026 06:52:05.996 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Last image: 2461237.82103720 16.07.2026 07:42:07.614 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10060
Objects passed selection criteria: 9991
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 5838
Average stars matched: 5674.5 (97.1994 %)
Memory usage VmPeak: 119688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 03:51:43 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461209.78629625 18.06.2026 06:52:05.996 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
First image: 2461209.78629625 18.06.2026 06:52:05.996 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Last image: 2461237.82103720 16.07.2026 07:42:07.614 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 108
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.09
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: 15 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): 67467
Objects passed selection criteria: 67254
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 42115
Average stars matched: 40554.5 (96.2947 %)
Memory usage VmPeak: 174480 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 03:54:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
SExtractor catalog cache: saved Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.cat to cache
SExtractor catalog cache: saved Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461237.82048227
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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits'
wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits exists and is non-empty
Saving wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits to local_wcs_cache/
'wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits' -> 'local_wcs_cache/wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits'
wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits'
wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits (1st reference image)
verification OK: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:19.676 +13:59:49.78 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-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits (1st new image)
verification OK: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:19.573 +13:59:57.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.676 +13:59:49.78
Second-epoch image center 16:53:19.573 +13:59:57.16
Angular distance between the image centers 0.0021 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits (2nd new image)
verification OK: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:22.435 +13:59:28.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:53:19.676 +13:59:49.78
Second-epoch image center 16:53:22.435 +13:59:28.99
Angular distance between the image centers 0.0126 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:53:19.573 +13:59:57.16
Second-epoch second image center 16:53:22.435 +13:59:28.99
Angular distance between the image centers 0.01397 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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits &> /tmp/tmp.Qn87A4Yoq7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits &> /tmp/tmp.tWpqsl3nNo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.eUbsJjRD3q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits &> /tmp/tmp.lj2buQIZ3v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
Found non-empty wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
The reference image (wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits) and catalog (wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat) found
'wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat' -> 'wcsmag.cat'
Read 13636 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.1104 to 261.5884 deg, Dec +8.6676 to +19.2473 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.1104 to 261.5884 deg, Dec 8.6676 to 19.2473 deg
Loaded 7645 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): 6255 out of 6563 total matches.
Matched with Tycho-2 6563 out of 13636 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777200
a=0.000000 b=1.000000 c=22.777200
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13636 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.1104 to 261.5884 deg, Dec +8.6676 to +19.2473 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.1104 to 261.5884 deg, Dec 8.6676 to 19.2473 deg
Loaded 7645 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): 6255 out of 6563 total matches.
Matched with Tycho-2 6563 out of 13636 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits:
Forced-photometry filter: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits -> calib.txt_param_ref_wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits (aperture=6.1)
Read 13632 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.1103 to 261.5883 deg, Dec +8.6686 to +19.2473 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.1103 to 261.5883 deg, Dec 8.6686 to 19.2473 deg
Loaded 7645 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): 6250 out of 6560 total matches.
Matched with Tycho-2 6560 out of 13632 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits:
Forced-photometry filter: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits -> calib.txt_param_ref_wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
2.2 pix Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
2.2 pix fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
2.3 pix fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
2.2 pix wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
2.2 pix wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Limiting magnitude estimates:
15.4 mag. Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
15.4 mag. Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
12.1 mag. fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
11.9 mag. fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 9.8 (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.Qn87A4Yoq7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits' -> 'wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Checking if the catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS catalog name: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=852, bad_region=2882, passed=13636
Got 13636 stars (including 10036 good ones) from the SExtractor catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
util/solve_plate_with_UCAC5 got 13636 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 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits N_match=978 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.422 n_q1=304 n_q2=186 n_q3=304 n_q4=184 worst_quadrant_to_overall_ratio=1.045
The image catalog is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits -region wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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.tWpqsl3nNo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits' -> 'wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Checking if the catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS catalog name: wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=834, bad_region=2878, passed=13632
Got 13632 stars (including 10059 good ones) from the SExtractor catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat
util/solve_plate_with_UCAC5 got 13632 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 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 11043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits N_match=978 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.450 n_q1=309 n_q2=186 n_q3=303 n_q4=180 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits -region wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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.eUbsJjRD3q (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=39, bad_region=107, passed=1058
Got 1058 stars (including 912 good ones) from the SExtractor catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 1058 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 547 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 493 to 547 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 884 stars left (next iteration limit 972)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits N_match=884 sigma_overall_arcsec=0.472 sigma_q1_arcsec=0.475 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.580 sigma_q4_arcsec=0.464 n_q1=268 n_q2=222 n_q3=199 n_q4=195 worst_quadrant_to_overall_ratio=1.229
The image catalog is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits -region wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.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.lj2buQIZ3v (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=38, bad_region=231, passed=1231
Got 1231 stars (including 966 good ones) from the SExtractor catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 1231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 1034 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 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 1031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 1031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits N_match=940 sigma_overall_arcsec=0.541 sigma_q1_arcsec=0.546 sigma_q2_arcsec=0.529 sigma_q3_arcsec=0.588 sigma_q4_arcsec=0.536 n_q1=302 n_q2=218 n_q3=209 n_q4=211 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits -region wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits sigma_overall=0.404 worst_q_ratio=1.045
ref2=Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits sigma_overall=0.407 worst_q_ratio=1.107
new1=fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits sigma_overall=0.472 worst_q_ratio=1.229
new2=fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits sigma_overall=0.541 worst_q_ratio=1.086
reference average sigma_overall=0.4055 worst_q_ratio=1.076
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222_astrometric_residuals.png (978 matched stars from wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223_astrometric_residuals.png (978 matched stars from wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226_astrometric_residuals.png (884 matched stars from wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227_astrometric_residuals.png (940 matched stars from wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits'
Preparing the HTML report for the field Her-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Her-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
SExtractor catalog cache: saved Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.cat to cache
SExtractor catalog cache: saved Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Creating symlink local_wcs_cache/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits exists and is non-empty
wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits exists and is non-empty
wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits (1st reference image)
verification OK: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:19.676 +13:59:49.78 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-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits (1st new image)
verification OK: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:19.573 +13:59:57.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.676 +13:59:49.78
Second-epoch image center 16:53:19.573 +13:59:57.16
Angular distance between the image centers 0.0021 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits (2nd new image)
verification OK: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:53:22.435 +13:59:28.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:53:19.676 +13:59:49.78
Second-epoch image center 16:53:22.435 +13:59:28.99
Angular distance between the image centers 0.0126 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:53:19.573 +13:59:57.16
Second-epoch second image center 16:53:22.435 +13:59:28.99
Angular distance between the image centers 0.01397 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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits &> /tmp/tmp.HJ6eyGxirJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits &> /tmp/tmp.twpB1G2RVU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.CAI9nZqRo0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits &> /tmp/tmp.Is5180j9Lk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
Found non-empty wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits and wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
The reference image (wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits) and catalog (wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat) found
'wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat' -> 'wcsmag.cat'
Read 86318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.0917 to 261.5884 deg, Dec +8.6676 to +19.2601 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.0917 to 261.5884 deg, Dec 8.6676 to 19.2601 deg
Loaded 7657 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): 5659 out of 6620 total matches.
Matched with Tycho-2 6620 out of 86318 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.634200
a=0.000000 b=1.000000 c=22.634200
From vast_summary.log: estimated ref. image limiting mag.: -7.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 86318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.0917 to 261.5884 deg, Dec +8.6676 to +19.2601 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.0917 to 261.5884 deg, Dec 8.6676 to 19.2601 deg
Loaded 7657 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): 5659 out of 6620 total matches.
Matched with Tycho-2 6620 out of 86318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits:
Forced-photometry filter: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits -> calib.txt_param_ref_wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits (aperture=4.6)
Read 85681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.0957 to 261.5883 deg, Dec +8.6686 to +19.2611 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.0957 to 261.5883 deg, Dec 8.6686 to 19.2611 deg
Loaded 7655 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): 5654 out of 6619 total matches.
Matched with Tycho-2 6619 out of 85681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits:
Forced-photometry filter: calibrated wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits -> calib.txt_param_ref_wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 106 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
2.1 pix Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
2.0 pix fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
2.1 pix fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
2.1 pix wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
2.1 pix wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Limiting magnitude estimates:
15.5 mag. Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
15.5 mag. Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
12.6 mag. fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
12.6 mag. fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.2 (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.HJ6eyGxirJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits' -> 'wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
Checking if the catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits
WCS catalog name: wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=5750, bad_region=11837, passed=86297
Got 86297 stars (including 69417 good ones) from the SExtractor catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat
util/solve_plate_with_UCAC5 got 86297 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 75560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 75560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 75560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits N_match=974 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.408 sigma_q4_arcsec=0.397 n_q1=288 n_q2=185 n_q3=306 n_q4=195 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits -region wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.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.twpB1G2RVU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits' -> 'wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
Checking if the catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat corresponding to the image wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits
WCS catalog name: wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=5638, bad_region=11744, passed=85663
Got 85663 stars (including 68947 good ones) from the SExtractor catalog wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat
util/solve_plate_with_UCAC5 got 85663 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 75155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 75156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 75156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits N_match=973 sigma_overall_arcsec=0.423 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.413 n_q1=285 n_q2=184 n_q3=310 n_q4=194 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits -region wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.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.CAI9nZqRo0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=224, bad_region=698, passed=11136
Got 11136 stars (including 10252 good ones) from the SExtractor catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 11136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 10313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 493 to 548 (Dec 8.6 to 19.3)
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(), 10314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 10314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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=fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits N_match=962 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.601 sigma_q4_arcsec=0.452 n_q1=301 n_q2=228 n_q3=226 n_q4=207 worst_quadrant_to_overall_ratio=1.289
The image catalog is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits -region wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.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.Is5180j9Lk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=244, bad_region=1456, passed=12136
Got 12136 stars (including 10496 good ones) from the SExtractor catalog wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 12136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
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(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 10850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
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: 965 matched stars entering correct_measured_positions(), 10850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 10850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits N_match=965 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.530 sigma_q2_arcsec=0.479 sigma_q3_arcsec=0.590 sigma_q4_arcsec=0.511 n_q1=324 n_q2=208 n_q3=222 n_q4=211 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits -region wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.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-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-41-19_20.00sec_5.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Her-09-Q2b1x1_024247_TTUQ2b1x1_1937703_UBTkQJUf/wcs_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227.fits
Preparing the HTML report for the field Her-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:50.02 +16:49:09.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:25.73 +13:09:18.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:40.32 +16:50:39.7: 13.17 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:42.59 +16:18:19.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:51.40 +10:54:42.5: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:04.58 +13:09:14.1: 11.91 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:37:59.87 +16:34:10.2: 13.49 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:50.02 +16:49:09.6: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:50.02 +16:49:09.6: ref_mag=12.97 +/- 0.02 new_mean_mag=11.9280 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:25.73 +13:09:18.2: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:25.73 +13:09:18.2: ref_mag=12.75 +/- 0.01 new_mean_mag=11.5462 delta=1.20 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:42.59 +16:18:19.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 16:38:42.59 +16:18:19.2: ref_mag=12.01 +/- 0.01 new_mean_mag=10.9594 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:04.58 +13:09:14.1: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:37:59.87 +16:34:10.2: 13.51 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:51.40 +10:54:42.5: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 17:20:04.58 +13:09:14.1: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9248 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 16:37:59.87 +16:34:10.2: ref_mag=13.50 +/- 0.02 new_mean_mag=12.4172 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 16:42:51.40 +10:54:42.5: ref_mag=13.49 +/- 0.02 new_mean_mag=12.1504 delta=1.34 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:06.52 +16:12:26.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:36.07 +10:36:58.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:40.32 +16:50:39.7: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 16:45:40.32 +16:50:39.7: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2186 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:29.99 +10:45:08.8: 13.28 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:36.07 +10:36:58.2: 13.27 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:06.52 +16:12:26.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 16:42:36.07 +10:36:58.2: ref_mag=13.27 +/- 0.02 new_mean_mag=12.1870 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:06.52 +16:12:26.3: ref_mag=13.30 +/- 0.02 new_mean_mag=12.0818 delta=1.22 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:29.99 +10:45:08.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 16:42:29.99 +10:45:08.8: ref_mag=13.29 +/- 0.02 new_mean_mag=12.1876 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:56.49 +13:23:52.4: 12.13 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:56.49 +13:23:52.4: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 17:20:56.49 +13:23:52.4: ref_mag=12.13 +/- 0.01 new_mean_mag=11.0965 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:56.22 +13:15:03.4: 12.11 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:56.22 +13:15:03.4: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 16:39:56.22 +13:15:03.4: ref_mag=12.13 +/- 0.01 new_mean_mag=11.1086 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:22.48 +13:18:59.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:30.60 +13:28:28.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:22.48 +13:18:59.4: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:11:11.47 +15:48:00.8: 12.62 +/- 0.01 detection
Forced photometry filter KEPT candidate at 17:21:22.48 +13:18:59.4: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6681 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:30.60 +13:28:28.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:30.60 +13:28:28.9: ref_mag=12.62 +/- 0.01 new_mean_mag=11.5600 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:11:11.47 +15:48:00.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 17:11:11.47 +15:48:00.8: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6811 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:12.40 +10:55:35.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:38.07 +13:36:11.6: 12.07 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:12.40 +10:55:35.0: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:22.05 +13:39:07.3: 13.26 +/- 0.03 detection
Forced photometry filter KEPT candidate at 16:42:12.40 +10:55:35.0: ref_mag=12.64 +/- 0.01 new_mean_mag=11.4857 delta=1.16 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:38.07 +13:36:11.6: 12.10 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:11.60 +12:34:19.0: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:38.07 +13:36:11.6: ref_mag=12.08 +/- 0.01 new_mean_mag=11.1162 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:22.05 +13:39:07.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:22.05 +13:39:07.3: ref_mag=13.25 +/- 0.02 new_mean_mag=12.1288 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:28.09 +16:11:09.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:11.60 +12:34:19.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 17:21:11.60 +12:34:19.0: ref_mag=12.97 +/- 0.02 new_mean_mag=11.9906 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:28.09 +16:11:09.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 16:40:28.09 +16:11:09.5: ref_mag=13.27 +/- 0.02 new_mean_mag=12.1894 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:42.36 +16:14:35.6: 13.25 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:42.36 +16:14:35.6: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 16:40:42.36 +16:14:35.6: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1755 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:33.44 +13:12:23.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:33.44 +13:12:23.6: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:33.44 +13:12:23.6: ref_mag=13.03 +/- 0.02 new_mean_mag=11.8520 delta=1.18 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:33.59 +10:52:39.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:33.59 +10:52:39.2: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 16:42:33.59 +10:52:39.2: ref_mag=12.97 +/- 0.01 new_mean_mag=11.7666 delta=1.21 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:50:34.02 +14:20:16.3: 13.21 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:50:34.02 +14:20:16.3: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 16:50:34.02 +14:20:16.3: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2411 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:52.79 +16:31:03.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:52.79 +16:31:03.0: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 16:45:52.79 +16:31:03.0: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2223 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:50.38 +16:39:58.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:50.38 +16:39:58.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 16:38:50.38 +16:39:58.8: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1483 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:50:48.91 +15:20:44.6: 13.16 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:13.21 +16:50:21.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:50:48.91 +15:20:44.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.01
Forced photometry filter KEPT candidate at 16:50:48.91 +15:20:44.6: ref_mag=13.13 +/- 0.01 new_mean_mag=12.0550 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:45:44.83 +16:47:32.6: 13.20 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:13.21 +16:50:21.2: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 16:40:13.21 +16:50:21.2: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2248 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:45:44.83 +16:47:32.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:43:00.03 +10:41:08.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 16:45:44.83 +16:47:32.6: ref_mag=13.17 +/- 0.02 new_mean_mag=12.2234 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:40.72 +10:48:45.9: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:04.30 +12:53:14.9: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:43:00.03 +10:41:08.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 16:43:00.03 +10:41:08.3: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9831 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:40.72 +10:48:45.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter KEPT candidate at 16:42:40.72 +10:48:45.9: ref_mag=11.91 +/- 0.01 new_mean_mag=10.9276 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:04.30 +12:53:14.9: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:04.30 +12:53:14.9: ref_mag=12.54 +/- 0.01 new_mean_mag=11.6219 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:02.99 +12:46:48.5: 12.53 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:02.99 +12:46:48.5: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:02.99 +12:46:48.5: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5939 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:36.81 +13:15:22.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:36.81 +13:15:22.9: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:36.81 +13:15:22.9: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6124 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:50.10 +16:51:39.5: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:50.10 +16:51:39.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:50.10 +16:51:39.5: ref_mag=13.43 +/- 0.02 new_mean_mag=12.3504 delta=1.08 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:46.34 +16:19:35.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:46.34 +16:19:35.3: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 16:38:46.34 +16:19:35.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.7852 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:37.21 +16:27:20.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:07.24 +16:28:21.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:37.21 +16:27:20.6: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:37.21 +16:27:20.6: ref_mag=13.43 +/- 0.02 new_mean_mag=12.0681 delta=1.36 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:07.24 +16:28:21.5: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 16:40:07.24 +16:28:21.5: ref_mag=12.89 +/- 0.01 new_mean_mag=11.7807 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:36:20.05 +12:05:34.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:36:20.05 +12:05:34.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 16:36:20.05 +12:05:34.2: ref_mag=13.41 +/- 0.02 new_mean_mag=12.2742 delta=1.13 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:16:28.86 +14:02:00.0: 13.82 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:12.90 +16:42:31.1: 12.54 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:16:28.86 +14:02:00.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 17:16:28.86 +14:02:00.0: ref_mag=13.80 +/- 0.03 new_mean_mag=12.2814 delta=1.52 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:50.61 +12:33:04.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:12.90 +16:42:31.1: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter KEPT candidate at 16:39:12.90 +16:42:31.1: ref_mag=12.53 +/- 0.01 new_mean_mag=11.4460 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:50.61 +12:33:04.9: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:50.61 +12:33:04.9: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5710 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:34.06 +16:36:12.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:34.06 +16:36:12.0: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:34.06 +16:36:12.0: ref_mag=13.42 +/- 0.02 new_mean_mag=12.1798 delta=1.24 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:17.27 +10:47:19.6: 13.17 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:17.27 +10:47:19.6: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 16:42:17.27 +10:47:19.6: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1602 delta=0.99 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:41:07.26 +10:04:55.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:41:07.26 +10:04:55.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 16:41:07.26 +10:04:55.6: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1572 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:49:30.77 +15:20:44.0: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:49:30.77 +15:20:44.0: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 16:49:30.77 +15:20:44.0: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0974 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:46.78 +13:27:15.2: 13.12 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:46.78 +13:27:15.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 17:19:46.78 +13:27:15.2: ref_mag=13.10 +/- 0.02 new_mean_mag=11.9797 delta=1.12 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:07.37 +16:27:06.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:59.32 +13:35:43.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:07.37 +16:27:06.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:07.37 +16:27:06.2: ref_mag=13.15 +/- 0.02 new_mean_mag=11.8149 delta=1.33 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:59.32 +13:35:43.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:59.32 +13:35:43.6: ref_mag=12.87 +/- 0.01 new_mean_mag=11.8483 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:21:27.74 +13:16:27.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:21:27.74 +13:16:27.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 17:21:27.74 +13:16:27.0: ref_mag=13.12 +/- 0.02 new_mean_mag=11.9744 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:46:08.79 +16:31:01.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:46:08.79 +16:31:01.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 16:46:08.79 +16:31:01.9: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1381 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:45.32 +16:50:00.0: 13.63 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:45.32 +16:50:00.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 16:38:45.32 +16:50:00.0: ref_mag=13.67 +/- 0.03 new_mean_mag=12.4491 delta=1.22 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:45.03 +16:40:45.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:45.03 +16:40:45.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 16:39:45.03 +16:40:45.2: ref_mag=12.87 +/- 0.01 new_mean_mag=11.7320 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:23.44 +13:06:25.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:23.44 +13:06:25.0: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:23.44 +13:06:25.0: ref_mag=12.80 +/- 0.01 new_mean_mag=11.5823 delta=1.22 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:19.84 +16:41:32.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:19.84 +16:41:32.4: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 16:38:19.84 +16:41:32.4: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3383 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:14.13 +16:25:39.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:14.13 +16:25:39.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:14.13 +16:25:39.0: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9395 delta=1.17 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:31.11 +13:08:45.3: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:31.11 +13:08:45.3: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:31.11 +13:08:45.3: ref_mag=12.32 +/- 0.01 new_mean_mag=11.2938 delta=1.02 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:45.37 +13:31:48.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:36:00.88 +12:03:53.9: 12.35 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:45.37 +13:31:48.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 17:18:45.37 +13:31:48.5: ref_mag=12.37 +/- 0.01 new_mean_mag=11.4051 delta=0.97 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:36:00.88 +12:03:53.9: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 16:36:00.88 +12:03:53.9: ref_mag=12.34 +/- 0.01 new_mean_mag=11.4056 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:35:13.71 +12:14:08.8: 12.77 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:35:13.71 +12:14:08.8: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 16:35:13.71 +12:14:08.8: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7018 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:16.63 +13:40:49.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:16.63 +13:40:49.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:16.63 +13:40:49.6: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7219 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:47:38.40 +17:22:31.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:47:38.40 +17:22:31.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 16:47:38.40 +17:22:31.9: ref_mag=13.03 +/- 0.01 new_mean_mag=12.0673 delta=0.96 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:43.44 +10:45:24.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:43.44 +10:45:24.2: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 16:42:43.44 +10:45:24.2: ref_mag=12.36 +/- 0.01 new_mean_mag=11.4344 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:35:11.99 +12:10:56.1: 13.36 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:35:11.99 +12:10:56.1: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 16:35:11.99 +12:10:56.1: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3365 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:36.87 +16:55:29.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:36.87 +16:55:29.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 16:38:36.87 +16:55:29.3: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0352 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:17.28 +16:48:26.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:17.28 +16:48:26.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:17.28 +16:48:26.7: ref_mag=13.38 +/- 0.02 new_mean_mag=12.2017 delta=1.18 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:33.56 +16:09:37.9: 13.56 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:04.38 +16:27:07.3: 13.58 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:41:11.19 +11:57:49.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:33.56 +16:09:37.9: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:33.56 +16:09:37.9: ref_mag=13.54 +/- 0.02 new_mean_mag=12.4763 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:09.78 +16:22:29.2: 13.61 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:04.38 +16:27:07.3: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 16:38:04.38 +16:27:07.3: ref_mag=13.55 +/- 0.02 new_mean_mag=12.2575 delta=1.29 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:41:11.19 +11:57:49.1: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 16:41:11.19 +11:57:49.1: ref_mag=13.57 +/- 0.03 new_mean_mag=12.3856 delta=1.19 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:09.78 +16:22:29.2: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 16:39:09.78 +16:22:29.2: ref_mag=13.64 +/- 0.02 new_mean_mag=12.3744 delta=1.27 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:21.21 +16:04:17.7: 13.56 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:21.21 +16:04:17.7: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 16:40:21.21 +16:04:17.7: ref_mag=13.57 +/- 0.02 new_mean_mag=12.4396 delta=1.13 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:01:39.61 +13:24:17.1: 12.70 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:01:39.61 +13:24:17.1: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 17:01:39.61 +13:24:17.1: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7970 delta=0.91 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:15.09 +13:09:35.6: 12.28 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:19.61 +13:24:07.7: 12.25 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:15.09 +13:09:35.6: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:15.09 +13:09:35.6: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2875 delta=0.98 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:19.61 +13:24:07.7: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:19.61 +13:24:07.7: ref_mag=12.24 +/- 0.01 new_mean_mag=11.2089 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:42:11.03 +10:55:02.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:42:11.03 +10:55:02.4: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 16:42:11.03 +10:55:02.4: ref_mag=13.03 +/- 0.01 new_mean_mag=11.7491 delta=1.28 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:18.05 +13:26:29.9: 13.55 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:18.05 +13:26:29.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 17:20:18.05 +13:26:29.9: ref_mag=13.49 +/- 0.03 new_mean_mag=12.2073 delta=1.28 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:39:28.61 +13:11:58.0: 12.24 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:18:31.88 +13:31:10.9: 13.29 +/- 0.03 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:39:28.61 +13:11:58.0: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter KEPT candidate at 16:39:28.61 +13:11:58.0: ref_mag=12.27 +/- 0.01 new_mean_mag=11.2260 delta=1.04 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:38:31.03 +16:32:43.5: 12.23 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:18:31.88 +13:31:10.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 17:18:31.88 +13:31:10.9: ref_mag=13.29 +/- 0.02 new_mean_mag=12.0646 delta=1.23 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 16:40:00.39 +13:16:02.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:38:31.03 +16:32:43.5: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 16:38:31.03 +16:32:43.5: ref_mag=12.24 +/- 0.01 new_mean_mag=11.1803 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:19:59.23 +13:29:53.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 16:40:00.39 +13:16:02.6: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 16:40:00.39 +13:16:02.6: ref_mag=13.67 +/- 0.03 new_mean_mag=12.3014 delta=1.37 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:19:59.23 +13:29:53.1: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 17:19:59.23 +13:29:53.1: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6588 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:22.44 +13:29:18.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:22.44 +13:29:18.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 17:20:22.44 +13:29:18.3: ref_mag=12.66 +/- 0.01 new_mean_mag=11.5118 delta=1.15 (need > 0.90)
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-05_20.00sec_4.90C_LIGHT_0222.fits at 17:20:41.04 +13:28:10.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_Her-09-Q2b1x1_2026-06-18_01-52-48_20.00sec_5.00C_LIGHT_0223.fits at 17:20:41.04 +13:28:10.8: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 17:20:41.04 +13:28:10.8: ref_mag=12.15 +/- 0.01 new_mean_mag=11.0488 delta=1.10 (need > 0.90)
Adding exclusion_list_local.txt__out102404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84085.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 123s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 60s
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Considering the candidate 102389_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 102389_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:03:11.63 +14:06:44.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102397_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 102397_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:02:57.71 +14:04:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102404_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 102404_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 42225_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 42225_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:29.49 +13:50:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48171_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48171_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 19466_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 19466_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 17598_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 17598_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48034_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48034_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 58646_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 58646_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 21649_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 21649_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 72257_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 72257_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 22518_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 22518_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 73443_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 73443_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 45915_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45915_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 42431_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 42431_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:22.76 +13:49:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47732_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 47732_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 45523_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 45523_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:18:02.80 +13:28:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46678_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 46678_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 45432_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45432_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 25742_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 25742_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 74767_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 74767_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 44023_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 44023_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 43858_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 43858_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 61946_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 61946_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 22792_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 22792_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 47660_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 47660_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:17.70 +13:13:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22301_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 22301_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48102_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48102_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 74524_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 74524_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 38679_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 38679_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20120_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20120_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 18781_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 18781_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 43428_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 43428_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:18:17.86 +13:42:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41634_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 41634_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:19.14 +13:55:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29961_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 29961_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 17485_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 17485_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 18023_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 18023_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 72952_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 72952_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 58566_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 58566_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 50484_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 50484_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 63588_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 63588_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 47257_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 47257_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 17343_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 17343_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 21540_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 21540_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20514_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20514_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20358_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20358_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 82503_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 82503_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 40095_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 40095_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:16:24.12 +14:06:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40792_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 40792_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 18417_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 18417_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 65910_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 65910_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48485_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 48485_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:20.96 +13:07:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19292_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 19292_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 73782_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 73782_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 68414_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 68414_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 29914_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 29914_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 45567_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45567_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20493_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20493_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 44377_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 44377_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 49019_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 49019_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:54.01 +13:03:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47058_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 47058_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20138_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20138_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 17474_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 17474_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 18683_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 18683_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48478_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48478_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 18515_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 18515_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 42726_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 42726_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:16.36 +13:47:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41497_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 41497_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:27.77 +13:56:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20660_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20660_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48219_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48219_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 44953_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 44953_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 83097_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 83097_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 84085_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 84085_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 47600_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 47600_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:50.95 +13:13:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43655_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 43655_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 13407_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 13407_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 73313_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 73313_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 47684_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 47684_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:47.67 +13:12:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83989_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 83989_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 16727_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 16727_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 17736_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 17736_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 40059_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 40059_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:16:56.18 +14:06:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43163_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 43163_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:18:02.79 +13:44:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67938_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 67938_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (51.1") between the two second-epoch detections
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Considering the candidate 22946_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 22946_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 20476_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 20476_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 81935_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 81935_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 21135_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 21135_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 23703_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 23703_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 46644_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 46644_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 48061_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48061_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 46020_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 46020_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 74348_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 74348_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45678_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45678_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41773_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 41773_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:16:53.71 +13:54:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45168_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45168_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48138_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 48138_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41451_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 41451_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:17:31.15 +13:56:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19574_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 19574_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47647_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 47647_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45256_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45256_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45228_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45228_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32549_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 32549_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 16:51:53.97 +14:56:29.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45342_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 45342_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45524_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 45524_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:18:17.99 +13:28:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34735_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227
The candidate 34735_fd_Her-09-Q2b1x1_2026-07-16_02-42-07_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 17:14:38.17 +14:23:26.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 190s
Prepared the HTML report for the field Her-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:39:50.02 +16:49:09.6
16:47:38.40 +17:22:31.9
16:38:36.87 +16:55:29.3
16:39:50.10 +16:51:39.5
16:38:45.32 +16:50:00.0
16:40:13.21 +16:50:21.2
16:45:40.32 +16:50:39.7
16:39:17.28 +16:48:26.7
16:45:44.83 +16:47:32.6
16:39:12.90 +16:42:31.1
16:38:19.84 +16:41:32.4
16:39:45.03 +16:40:45.2
16:38:50.38 +16:39:58.8
16:39:34.06 +16:36:12.0
16:37:59.87 +16:34:10.2
16:38:31.03 +16:32:43.5
16:45:52.79 +16:31:03.0
16:46:08.79 +16:31:01.9
16:40:07.24 +16:28:21.5
16:38:04.38 +16:27:07.3
16:39:07.37 +16:27:06.2
16:39:37.21 +16:27:20.6
16:39:14.13 +16:25:39.0
16:39:09.78 +16:22:29.2
16:38:46.34 +16:19:35.3
16:38:42.59 +16:18:19.2
16:40:42.36 +16:14:35.6
16:39:06.52 +16:12:26.3
16:40:28.09 +16:11:09.5
16:39:33.56 +16:09:37.9
16:40:21.21 +16:04:17.7
17:11:11.47 +15:48:00.8
16:49:30.77 +15:20:44.0
16:50:48.91 +15:20:44.6
16:50:34.02 +14:20:16.3
17:16:28.86 +14:02:00.0
17:19:16.63 +13:40:49.6
17:19:22.05 +13:39:07.3
17:18:38.07 +13:36:11.6
17:18:59.32 +13:35:43.6
17:18:45.37 +13:31:48.5
17:18:31.88 +13:31:10.9
17:20:22.44 +13:29:18.3
17:19:59.23 +13:29:53.1
17:20:41.04 +13:28:10.8
17:19:30.60 +13:28:28.9
17:19:46.78 +13:27:15.2
17:20:18.05 +13:26:29.9
17:20:56.49 +13:23:52.4
17:19:19.61 +13:24:07.7
17:01:39.61 +13:24:17.1
17:21:22.48 +13:18:59.4
17:21:27.74 +13:16:27.0
17:18:36.81 +13:15:22.9
16:40:00.39 +13:16:02.6
16:39:56.22 +13:15:03.4
17:20:04.58 +13:09:14.1
17:19:15.09 +13:09:35.6
16:39:33.44 +13:12:23.6
16:39:28.61 +13:11:58.0
17:18:25.73 +13:09:18.2
17:18:31.11 +13:08:45.3
17:18:23.44 +13:06:25.0
17:19:04.30 +12:53:14.9
16:42:40.72 +10:48:45.9
16:42:51.40 +10:54:42.5
17:21:11.60 +12:34:19.0
17:19:02.99 +12:46:48.5
17:18:50.61 +12:33:04.9
16:41:07.26 +10:04:55.6
16:42:36.07 +10:36:58.2
16:43:00.03 +10:41:08.3
16:42:43.44 +10:45:24.2
16:42:29.99 +10:45:08.8
16:42:17.27 +10:47:19.6
16:42:11.03 +10:55:02.4
16:42:33.59 +10:52:39.2
16:42:12.40 +10:55:35.0
16:41:11.19 +11:57:49.1
16:36:20.05 +12:05:34.2
16:36:00.88 +12:03:53.9
16:35:11.99 +12:10:56.1
16:35:13.71 +12:14:08.8
########### Completed Her-09-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
16:39:50.02 +16:49:09.6
17:18:25.73 +13:09:18.2
16:37:59.87 +16:34:10.2
16:45:40.32 +16:50:39.7
17:20:04.58 +13:09:14.1
16:42:51.40 +10:54:42.5
16:38:42.59 +16:18:19.2
16:42:36.07 +10:36:58.2
16:39:06.52 +16:12:26.3
16:42:29.99 +10:45:08.8
17:20:56.49 +13:23:52.4
16:39:56.22 +13:15:03.4
17:21:22.48 +13:18:59.4
17:19:30.60 +13:28:28.9
17:11:11.47 +15:48:00.8
16:42:12.40 +10:55:35.0
17:18:38.07 +13:36:11.6
17:19:22.05 +13:39:07.3
17:21:11.60 +12:34:19.0
16:40:28.09 +16:11:09.5
16:40:42.36 +16:14:35.6
16:39:33.44 +13:12:23.6
16:42:33.59 +10:52:39.2
16:50:34.02 +14:20:16.3
16:45:52.79 +16:31:03.0
16:38:50.38 +16:39:58.8
16:50:48.91 +15:20:44.6
16:40:13.21 +16:50:21.2
16:45:44.83 +16:47:32.6
16:43:00.03 +10:41:08.3
16:42:40.72 +10:48:45.9
17:19:04.30 +12:53:14.9
17:19:02.99 +12:46:48.5
17:18:36.81 +13:15:22.9
16:39:50.10 +16:51:39.5
16:38:46.34 +16:19:35.3
16:39:37.21 +16:27:20.6
16:40:07.24 +16:28:21.5
16:36:20.05 +12:05:34.2
17:16:28.86 +14:02:00.0
16:39:12.90 +16:42:31.1
17:18:50.61 +12:33:04.9
16:39:34.06 +16:36:12.0
16:42:17.27 +10:47:19.6
16:41:07.26 +10:04:55.6
16:49:30.77 +15:20:44.0
17:19:46.78 +13:27:15.2
16:39:07.37 +16:27:06.2
17:18:59.32 +13:35:43.6
17:21:27.74 +13:16:27.0
16:46:08.79 +16:31:01.9
16:38:45.32 +16:50:00.0
16:39:45.03 +16:40:45.2
17:18:23.44 +13:06:25.0
16:38:19.84 +16:41:32.4
16:39:14.13 +16:25:39.0
17:18:31.11 +13:08:45.3
17:18:45.37 +13:31:48.5
16:36:00.88 +12:03:53.9
16:35:13.71 +12:14:08.8
17:19:16.63 +13:40:49.6
16:47:38.40 +17:22:31.9
16:42:43.44 +10:45:24.2
16:35:11.99 +12:10:56.1
16:38:36.87 +16:55:29.3
16:39:17.28 +16:48:26.7
16:39:33.56 +16:09:37.9
16:38:04.38 +16:27:07.3
16:41:11.19 +11:57:49.1
16:39:09.78 +16:22:29.2
16:40:21.21 +16:04:17.7
17:01:39.61 +13:24:17.1
17:19:15.09 +13:09:35.6
17:19:19.61 +13:24:07.7
16:42:11.03 +10:55:02.4
17:20:18.05 +13:26:29.9
17:18:31.88 +13:31:10.9
16:39:28.61 +13:11:58.0
16:38:31.03 +16:32:43.5
16:40:00.39 +13:16:02.6
17:19:59.23 +13:29:53.1
17:20:22.44 +13:29:18.3
17:20:41.04 +13:28:10.8
###################################################################################
16:39:50.02 +16:49:09.6 -- not an asteroid (will add it to exclusion list)
17:18:25.73 +13:09:18.2 -- not an asteroid (will add it to exclusion list)
16:37:59.87 +16:34:10.2 -- not an asteroid (will add it to exclusion list)
16:45:40.32 +16:50:39.7 -- not an asteroid (will add it to exclusion list)
17:20:04.58 +13:09:14.1 -- not an asteroid (will add it to exclusion list)
16:42:51.40 +10:54:42.5 -- not an asteroid (will add it to exclusion list)
16:38:42.59 +16:18:19.2 -- not an asteroid (will add it to exclusion list)
16:42:36.07 +10:36:58.2 -- not an asteroid (will add it to exclusion list)
16:39:06.52 +16:12:26.3 -- not an asteroid (will add it to exclusion list)
16:42:29.99 +10:45:08.8 -- not an asteroid (will add it to exclusion list)
17:20:56.49 +13:23:52.4 -- not an asteroid (will add it to exclusion list)
16:39:56.22 +13:15:03.4 -- not an asteroid (will add it to exclusion list)
17:21:22.48 +13:18:59.4 -- not an asteroid (will add it to exclusion list)
17:19:30.60 +13:28:28.9 -- not an asteroid (will add it to exclusion list)
17:11:11.47 +15:48:00.8 -- not an asteroid (will add it to exclusion list)
16:42:12.40 +10:55:35.0 -- not an asteroid (will add it to exclusion list)
17:18:38.07 +13:36:11.6 -- not an asteroid (will add it to exclusion list)
17:19:22.05 +13:39:07.3 -- not an asteroid (will add it to exclusion list)
17:21:11.60 +12:34:19.0 -- not an asteroid (will add it to exclusion list)
16:40:28.09 +16:11:09.5 -- not an asteroid (will add it to exclusion list)
16:40:42.36 +16:14:35.6 -- not an asteroid (will add it to exclusion list)
16:39:33.44 +13:12:23.6 -- not an asteroid (will add it to exclusion list)
16:42:33.59 +10:52:39.2 -- not an asteroid (will add it to exclusion list)
16:50:34.02 +14:20:16.3 -- not an asteroid (will add it to exclusion list)
16:45:52.79 +16:31:03.0 -- not an asteroid (will add it to exclusion list)
16:38:50.38 +16:39:58.8 -- not an asteroid (will add it to exclusion list)
16:50:48.91 +15:20:44.6 -- not an asteroid (will add it to exclusion list)
16:40:13.21 +16:50:21.2 -- not an asteroid (will add it to exclusion list)
16:45:44.83 +16:47:32.6 -- not an asteroid (will add it to exclusion list)
16:43:00.03 +10:41:08.3 -- not an asteroid (will add it to exclusion list)
16:42:40.72 +10:48:45.9 -- not an asteroid (will add it to exclusion list)
17:19:04.30 +12:53:14.9 -- not an asteroid (will add it to exclusion list)
17:19:02.99 +12:46:48.5 -- not an asteroid (will add it to exclusion list)
17:18:36.81 +13:15:22.9 -- not an asteroid (will add it to exclusion list)
16:39:50.10 +16:51:39.5 -- not an asteroid (will add it to exclusion list)
16:38:46.34 +16:19:35.3 -- not an asteroid (will add it to exclusion list)
16:39:37.21 +16:27:20.6 -- not an asteroid (will add it to exclusion list)
16:40:07.24 +16:28:21.5 -- not an asteroid (will add it to exclusion list)
16:36:20.05 +12:05:34.2 -- not an asteroid (will add it to exclusion list)
17:16:28.86 +14:02:00.0 -- not an asteroid (will add it to exclusion list)
16:39:12.90 +16:42:31.1 -- not an asteroid (will add it to exclusion list)
17:18:50.61 +12:33:04.9 -- not an asteroid (will add it to exclusion list)
16:39:34.06 +16:36:12.0 -- not an asteroid (will add it to exclusion list)
16:42:17.27 +10:47:19.6 -- not an asteroid (will add it to exclusion list)
16:41:07.26 +10:04:55.6 -- not an asteroid (will add it to exclusion list)
16:49:30.77 +15:20:44.0 -- not an asteroid (will add it to exclusion list)
17:19:46.78 +13:27:15.2 -- not an asteroid (will add it to exclusion list)
16:39:07.37 +16:27:06.2 -- not an asteroid (will add it to exclusion list)
17:18:59.32 +13:35:43.6 -- not an asteroid (will add it to exclusion list)
17:21:27.74 +13:16:27.0 -- not an asteroid (will add it to exclusion list)
16:46:08.79 +16:31:01.9 -- not an asteroid (will add it to exclusion list)
16:38:45.32 +16:50:00.0 -- not an asteroid (will add it to exclusion list)
16:39:45.03 +16:40:45.2 -- not an asteroid (will add it to exclusion list)
17:18:23.44 +13:06:25.0 -- not an asteroid (will add it to exclusion list)
16:38:19.84 +16:41:32.4 -- not an asteroid (will add it to exclusion list)
16:39:14.13 +16:25:39.0 -- not an asteroid (will add it to exclusion list)
17:18:31.11 +13:08:45.3 -- not an asteroid (will add it to exclusion list)
17:18:45.37 +13:31:48.5 -- not an asteroid (will add it to exclusion list)
16:36:00.88 +12:03:53.9 -- not an asteroid (will add it to exclusion list)
16:35:13.71 +12:14:08.8 -- not an asteroid (will add it to exclusion list)
17:19:16.63 +13:40:49.6 -- not an asteroid (will add it to exclusion list)
16:47:38.40 +17:22:31.9 -- not an asteroid (will add it to exclusion list)
16:42:43.44 +10:45:24.2 -- not an asteroid (will add it to exclusion list)
16:35:11.99 +12:10:56.1 -- not an asteroid (will add it to exclusion list)
16:38:36.87 +16:55:29.3 -- not an asteroid (will add it to exclusion list)
16:39:17.28 +16:48:26.7 -- not an asteroid (will add it to exclusion list)
16:39:33.56 +16:09:37.9 -- not an asteroid (will add it to exclusion list)
16:38:04.38 +16:27:07.3 -- not an asteroid (will add it to exclusion list)
16:41:11.19 +11:57:49.1 -- not an asteroid (will add it to exclusion list)
16:39:09.78 +16:22:29.2 -- not an asteroid (will add it to exclusion list)
16:40:21.21 +16:04:17.7 -- not an asteroid (will add it to exclusion list)
17:01:39.61 +13:24:17.1 -- not an asteroid (will add it to exclusion list)
17:19:15.09 +13:09:35.6 -- not an asteroid (will add it to exclusion list)
17:19:19.61 +13:24:07.7 -- not an asteroid (will add it to exclusion list)
16:42:11.03 +10:55:02.4 -- not an asteroid (will add it to exclusion list)
17:20:18.05 +13:26:29.9 -- not an asteroid (will add it to exclusion list)
17:18:31.88 +13:31:10.9 -- not an asteroid (will add it to exclusion list)
16:39:28.61 +13:11:58.0 -- not an asteroid (will add it to exclusion list)
16:38:31.03 +16:32:43.5 -- not an asteroid (will add it to exclusion list)
16:40:00.39 +13:16:02.6 -- not an asteroid (will add it to exclusion list)
17:19:59.23 +13:29:53.1 -- not an asteroid (will add it to exclusion list)
17:20:22.44 +13:29:18.3 -- not an asteroid (will add it to exclusion list)
17:20:41.04 +13:28:10.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:35:11.99 +12:10:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:13.71 +12:14:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:00.88 +12:03:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:20.05 +12:05:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:59.87 +16:34:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:04.38 +16:27:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:19.84 +16:41:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:31.03 +16:32:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:36.87 +16:55:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:42.59 +16:18:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:45.32 +16:50:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:46.34 +16:19:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:50.38 +16:39:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:06.52 +16:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:07.37 +16:27:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:09.78 +16:22:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:12.90 +16:42:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:14.13 +16:25:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:17.28 +16:48:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:28.61 +13:11:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:33.44 +13:12:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:33.56 +16:09:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:34.06 +16:36:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:37.21 +16:27:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:45.03 +16:40:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:50.02 +16:49:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:50.10 +16:51:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:56.22 +13:15:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:00.39 +13:16:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:07.24 +16:28:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:13.21 +16:50:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:21.21 +16:04:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:28.09 +16:11:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:42.36 +16:14:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:07.26 +10:04:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:11.19 +11:57:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:11.03 +10:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:12.40 +10:55:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:17.27 +10:47:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:29.99 +10:45:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:33.59 +10:52:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:36.07 +10:36:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:40.72 +10:48:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:43.44 +10:45:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:51.40 +10:54:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:00.03 +10:41:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:40.32 +16:50:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:44.83 +16:47:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:52.79 +16:31:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:08.79 +16:31:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:38.40 +17:22:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:30.77 +15:20:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:34.02 +14:20:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:48.91 +15:20:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:39.61 +13:24:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:11:11.47 +15:48:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:28.86 +14:02:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:23.44 +13:06:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:25.73 +13:09:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:31.11 +13:08:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:31.88 +13:31:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:36.81 +13:15:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:38.07 +13:36:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:45.37 +13:31:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:50.61 +12:33:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:18:59.32 +13:35:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:02.99 +12:46:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:04.30 +12:53:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:15.09 +13:09:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:16.63 +13:40:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:19.61 +13:24:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:22.05 +13:39:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:30.60 +13:28:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:46.78 +13:27:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:59.23 +13:29:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:04.58 +13:09:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:18.05 +13:26:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:22.44 +13:29:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:41.04 +13:28:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:20:56.49 +13:23:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:11.60 +12:34:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:22.48 +13:18:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:27.74 +13:16:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
16:35:11.99 +12:10:56.1 -- not a known variable star
16:35:13.71 +12:14:08.8 -- not a known variable star
16:36:00.88 +12:03:53.9 -- not a known variable star
16:36:20.05 +12:05:34.2 -- not a known variable star
16:37:59.87 +16:34:10.2 -- not a known variable star
16:38:04.38 +16:27:07.3 -- not a known variable star
16:38:19.84 +16:41:32.4 -- not a known variable star
16:38:31.03 +16:32:43.5 -- not a known variable star
16:38:36.87 +16:55:29.3 -- not a known variable star
16:38:42.59 +16:18:19.2 -- not a known variable star
16:38:45.32 +16:50:00.0 -- not a known variable star
16:38:46.34 +16:19:35.3 -- not a known variable star
16:38:50.38 +16:39:58.8 -- a known variable star
16:39:06.52 +16:12:26.3 -- not a known variable star
16:39:07.37 +16:27:06.2 -- not a known variable star
16:39:09.78 +16:22:29.2 -- not a known variable star
16:39:12.90 +16:42:31.1 -- not a known variable star
16:39:14.13 +16:25:39.0 -- not a known variable star
16:39:17.28 +16:48:26.7 -- not a known variable star
16:39:28.61 +13:11:58.0 -- not a known variable star
16:39:33.44 +13:12:23.6 -- not a known variable star
16:39:33.56 +16:09:37.9 -- not a known variable star
16:39:34.06 +16:36:12.0 -- not a known variable star
16:39:37.21 +16:27:20.6 -- not a known variable star
16:39:45.03 +16:40:45.2 -- not a known variable star
16:39:50.02 +16:49:09.6 -- a known variable star
16:39:50.10 +16:51:39.5 -- not a known variable star
16:39:56.22 +13:15:03.4 -- not a known variable star
16:40:00.39 +13:16:02.6 -- not a known variable star
16:40:07.24 +16:28:21.5 -- not a known variable star
16:40:13.21 +16:50:21.2 -- not a known variable star
16:40:21.21 +16:04:17.7 -- not a known variable star
16:40:28.09 +16:11:09.5 -- not a known variable star
16:40:42.36 +16:14:35.6 -- not a known variable star
16:41:07.26 +10:04:55.6 -- not a known variable star
16:41:11.19 +11:57:49.1 -- not a known variable star
16:42:11.03 +10:55:02.4 -- not a known variable star
16:42:12.40 +10:55:35.0 -- not a known variable star
16:42:17.27 +10:47:19.6 -- not a known variable star
16:42:29.99 +10:45:08.8 -- not a known variable star
16:42:33.59 +10:52:39.2 -- a known variable star
16:42:36.07 +10:36:58.2 -- not a known variable star
16:42:40.72 +10:48:45.9 -- not a known variable star
16:42:43.44 +10:45:24.2 -- not a known variable star
16:42:51.40 +10:54:42.5 -- not a known variable star
16:43:00.03 +10:41:08.3 -- not a known variable star
16:45:40.32 +16:50:39.7 -- not a known variable star
16:45:44.83 +16:47:32.6 -- not a known variable star
16:45:52.79 +16:31:03.0 -- not a known variable star
16:46:08.79 +16:31:01.9 -- a known variable star
16:47:38.40 +17:22:31.9 -- not a known variable star
16:49:30.77 +15:20:44.0 -- not a known variable star
16:50:34.02 +14:20:16.3 -- not a known variable star
16:50:48.91 +15:20:44.6 -- a known variable star
17:01:39.61 +13:24:17.1 -- not a known variable star
17:11:11.47 +15:48:00.8 -- not a known variable star
17:16:28.86 +14:02:00.0 -- not a known variable star
17:18:23.44 +13:06:25.0 -- not a known variable star
17:18:25.73 +13:09:18.2 -- not a known variable star
17:18:31.11 +13:08:45.3 -- not a known variable star
17:18:31.88 +13:31:10.9 -- not a known variable star
17:18:36.81 +13:15:22.9 -- not a known variable star
17:18:38.07 +13:36:11.6 -- not a known variable star
17:18:45.37 +13:31:48.5 -- not a known variable star
17:18:50.61 +12:33:04.9 -- not a known variable star
17:18:59.32 +13:35:43.6 -- not a known variable star
17:19:02.99 +12:46:48.5 -- not a known variable star
17:19:04.30 +12:53:14.9 -- not a known variable star
17:19:15.09 +13:09:35.6 -- not a known variable star
17:19:16.63 +13:40:49.6 -- not a known variable star
17:19:19.61 +13:24:07.7 -- not a known variable star
17:19:22.05 +13:39:07.3 -- not a known variable star
17:19:30.60 +13:28:28.9 -- not a known variable star
17:19:46.78 +13:27:15.2 -- not a known variable star
17:19:59.23 +13:29:53.1 -- not a known variable star
17:20:04.58 +13:09:14.1 -- not a known variable star
17:20:18.05 +13:26:29.9 -- not a known variable star
17:20:22.44 +13:29:18.3 -- not a known variable star
17:20:41.04 +13:28:10.8 -- not a known variable star
17:20:56.49 +13:23:52.4 -- a known variable star
17:21:11.60 +12:34:19.0 -- not a known variable star
17:21:22.48 +13:18:59.4 -- not a known variable star
17:21:27.74 +13:16:27.0 -- not a known variable star
Found 77 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
83 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 83 (excluding asteroids and hot pixels, 77 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461237.82048227 -observatory V36
07:16:39.47 +17:17:59.4 Mercury (4.8mag)
10:36:14.65 +09:59:51.1 Venus (-4.1mag)
04:41:52.25 +22:06:27.7 Mars (1.3mag)
08:22:06.64 +19:54:02.7 Jupiter (-1.8mag)
00:56:23.76 +03:22:06.3 Saturn (0.7mag)
04:08:20.35 +20:48:01.6 Uranus (5.8mag)
00:16:57.77 +00:19:56.6 Neptune (7.7mag)
20:30:21.49 -23:20:38.2 Pluto (14.4mag)
09:29:12.70 +14:59:22.3 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 361 Jul 16 03:51 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461237.82048227:
08:22:06.97 +19:54:00.8 Io (6.0mag)
08:21:58.31 +19:54:35.3 Europa (6.3mag)
08:22:12.20 +19:53:45.8 Ganymede (5.6mag)
08:21:43.70 +19:55:27.5 Callisto (6.8mag)
08:20:22.26 +19:40:50.1 Himalia (15.7mag)
08:22:04.71 +19:54:11.2 Thebe (16.6mag)
08:19:43.02 +19:43:59.0 Elara (17.7mag)
08:25:49.37 +19:45:01.9 Pasiphae (17.9mag)
08:26:43.77 +20:00:01.1 Carme (19.0mag)
00:56:35.65 +03:21:51.6 Titan (8.5mag)
00:56:25.85 +03:21:51.3 Rhea (9.8mag)
00:55:48.97 +03:20:12.7 Iapetus (11.2mag)
00:56:10.43 +03:22:18.0 Hyperion (14.5mag)
00:56:16.50 +03:18:27.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 03:51 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.82048227:
17:55:00.46 -31:35:47.1 JWST
17:40:24.13 +36:05:41.3 Chandra
02:21:55.66 +63:02:46.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 03:51 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.82048227 -observatory V36
02:44:39.13 +15:07:22.1 17.8mag P/1996 R2 (Lagerkvist)
18:13:30.34 -34:30:27.4 13.8mag P/2010 H2 (Vales)
06:31:38.16 -68:14:41.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:51.33 +32:33:00.5 17.6mag C/2017 K2 (PANSTARRS)
02:19:08.16 +18:33:22.9 15.7mag P/2021 N1 (ZTF)
22:55:48.48 +32:15:02.3 17.3mag C/2022 E2 (ATLAS)
06:19:09.65 +26:52:07.1 16.7mag C/2022 N2 (PANSTARRS)
10:00:45.13 +29:30:44.9 16.9mag C/2022 QE78 (ATLAS)
09:13:36.67 +05:06:15.1 17.9mag C/2022 R6 (PANSTARRS)
18:03:39.53 +21:02:41.4 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.43 -11:31:58.3 17.8mag P/2023 B1 (PANSTARRS)
21:41:48.90 +67:32:15.5 17.8mag C/2023 H5 (Lemmon)
16:19:36.33 -10:41:51.3 14.0mag C/2023 R1 (PANSTARRS)
08:11:07.60 +66:02:13.8 17.9mag C/2024 A1 (ATLAS)
07:40:33.39 +30:18:04.0 14.8mag C/2024 E1 (Wierzchos)
15:13:36.25 +15:27:58.3 17.6mag C/2024 G6 (ATLAS)
19:33:34.88 +40:29:36.0 13.7mag C/2024 J3 (ATLAS)
21:41:08.41 +46:52:09.0 17.8mag C/2024 R4 (PANSTARRS)
04:55:13.74 -13:32:32.1 15.7mag C/2024 T5 (ATLAS)
06:39:27.42 +28:04:23.1 18.0mag C/2025 J1 (Borisov)
07:18:24.28 -13:26:28.6 16.8mag C/2025 R3 (PANSTARRS)
10:03:07.93 +22:10:14.8 17.6mag C/2025 V2 (Rankin)
12:46:45.08 +03:40:11.1 17.1mag C/2025 Y1 (ATLAS)
16:35:49.26 +79:09:31.7 17.2mag C/2026 A2 (Bok)
02:52:19.05 +45:29:22.6 16.8mag C/2026 B2 (Sun-Gao)
11:29:25.56 +05:33:33.0 17.0mag A/2026 E1
21:28:14.89 -17:19:23.9 7.1mag 10P/Tempel
11:16:19.68 -02:09:08.2 16.2mag 29P/Schwassmann-Wachmann
04:08:42.81 +30:11:38.2 17.9mag 47P/Ashbrook-Jackson
10:20:31.66 +12:06:05.1 17.1mag 63P/Wild
00:50:44.49 -05:02:51.8 15.5mag 65P/Gunn
04:41:48.54 +20:27:19.8 13.7mag 78P/Gehrels
02:31:45.09 +11:24:14.1 16.3mag 88P/Howell
06:53:08.91 +30:08:16.9 15.8mag 93P/Lovas
04:40:29.00 +31:18:27.8 16.7mag 114P/Wiseman-Skiff
08:23:16.73 +30:00:36.0 15.2mag 123P/West-Hartley
10:59:19.20 -01:14:02.8 16.9mag 124P/Mrkos
05:01:17.20 +20:58:07.2 16.2mag 128P/Shoemaker-Holt
05:47:27.79 +19:38:49.4 17.8mag 131P/Mueller
00:02:58.28 +03:08:52.1 17.9mag 139P/Vaisala-Oterma
07:35:02.04 +15:42:09.5 16.3mag 141P-D/Machholz
03:19:09.93 -20:37:46.6 15.2mag 161P/Hartley-IRAS
05:54:35.97 +35:09:05.7 15.4mag 162P/SidingSpring
18:46:42.30 +19:02:29.1 14.2mag 169P/NEAT
01:55:06.29 +08:13:40.3 17.6mag 220P/McNaught
16:35:30.12 -08:38:43.5 17.2mag 235P/LINEAR
08:57:48.15 +32:44:04.0 18.0mag 240P/NEAT
20:39:10.04 -50:47:47.4 17.8mag 259P/Garradd
02:16:05.63 +14:53:05.7 15.6mag 260P/McNaught
05:55:23.77 +37:16:25.3 17.4mag 295P/LINEAR
15:06:29.44 +05:30:40.6 17.6mag 391P/Kowalski
08:39:59.05 +19:25:47.3 17.9mag 450P/LONEOS
08:01:06.37 +38:43:01.7 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 03:51 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 16 03:51 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 16 03:51 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:58:49.786 -21:29:54.27 AT 2026ssv 2026-07-06.26 21.93
21:15:32.626 -21:37:53.76 AT 2026ssu 2026-06-27.33 21.39
22:49:45.273 -15:16:33.71 AT 2026sst 2026-06-27.41 21.88
22:21:22.865 -18:28:38.60 AT 2026sss 2026-06-26.37 22.73
21:48:11.294 -15:58:33.77 AT 2026ssr 2026-06-26.41 21.95
21:56:29.244 -10:33:36.38 AT 2026ssq 2026-06-26.39 22.31
22:04:36.634 -18:37:38.63 AT 2026ssp 2026-06-26.37 22.56
21:52:03.725 -20:04:23.97 AT 2026sso 2026-06-26.39 22.15
22:28:31.768 -14:13:03.02 AT 2026ssn 2026-06-26.40 23.19
22:10:38.868 -20:00:07.81 AT 2026ssm 2026-06-26.37 21.5
00:37:08.843 -05:37:20.31 AT 2026ssl 2026-06-23.58 20.49
16:50:39.367 +12:02:04.48 AT 2026ssk 2026-06-23.30 21.04
21:28:51.588 -30:52:46.37 AT 2026ssj 2026-06-23.54 20.48
13:14:31.067 +38:32:01.92 AT 2026ssi 2026-06-11.32 19.048
00:23:13.025 -04:43:14.99 AT 2026ssh 2026-06-23.58 20.7
21:26:53.186 +04:17:24.51 AT 2026ssg 2026-06-23.48 20.92
22:34:24.397 -29:59:37.51 AT 2026ssf 2026-06-25.56 20.68
22:26:15.310 -27:42:10.55 AT 2026sse 2026-06-25.56 21.41
22:13:00.422 -28:48:04.48 AT 2026ssd 2026-06-25.55 21.47
22:13:31.243 -26:34:31.26 AT 2026ssc 2026-06-25.55 21.32
-rw-r--r-- 1 apache apache 89K Jul 16 03:51 tns_transients_list.txt
