This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.46 02:18:43.76 +32:27:54.6
143.52165 -26.89274 galactic Tri Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:43.76 +32:27:54.6 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:43.76 +32:27:54.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:43.76 +32:27:54.6: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 18 43.76 +32 27 54.6 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.46,0.05,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 20260710.3317 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.21 02:18:52.39 +32:23:56.6
143.58079 -26.94285 galactic Tri Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:52.39 +32:23:56.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.712+/-0.030 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:52.39 +32:23:56.6: 13.10 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:52.39 +32:23:56.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 18 52.39 +32 23 56.6 12.2 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.52 02:19:37.66 +30:22:24.6
144.61179 -28.75888 galactic Tri Second-epoch detections are separated by 0.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:37.66 +30:22:24.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.474+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:37.66 +30:22:24.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:37.66 +30:22:24.6: 13.52 +/- 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 10.3316* 02 19 37.66 +30 22 24.6 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.52,0.05,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 20260710.3317 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.04 02:20:54.45 +31:58:37.3
144.20688 -27.17195 galactic Tri Second-epoch detections are separated by 0.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:54.45 +31:58:37.3 (user input) | T | P | (position from user input) J-Ks=0.637+/-0.024 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:54.45 +31:58:37.3: 12.94 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:54.45 +31:58:37.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 54.45 +31 58 37.3 12.0 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.88 01:51:19.97 +28:28:38.1
138.56618 -32.56963 galactic Tri Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:51:19.97 +28:28:38.1 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:51:19.97 +28:28:38.1: 13.88 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:51:19.97 +28:28:38.1: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 01 51 19.97 +28 28 38.1 12.9 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.88,0.05,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 20260710.3317 12.88CV 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 10.3317 2461231.8317 12.15 02:19:25.93 +31:06:18.0
144.25192 -28.09804 galactic Tri Second-epoch detections are separated by 4.1" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:25.93 +31:06:18.0 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.846+/-0.027 (M)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:25.93 +31:06:18.0: 13.23 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:25.93 +31:06:18.0: 13.22 +/- 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 10.3316* 02 19 25.93 +31 06 18.0 12.2 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.15,0.05,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 20260710.3317 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.23 02:20:54.79 +31:08:26.2
144.56858 -27.94446 galactic Tri Second-epoch detections are separated by 0.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:54.79 +31:08:26.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.466+/-0.029 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:54.79 +31:08:26.2: 13.21 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:54.79 +31:08:26.2: 13.23 +/- 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 10.3316* 02 20 54.79 +31 08 26.2 12.2 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.23,0.05,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 20260710.3317 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 10.3317 2461231.8317 12.21 02:19:29.97 +30:46:30.0
144.40892 -28.39801 galactic Tri Second-epoch detections are separated by 0.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:29.97 +30:46:30.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.979+/-0.029 (M)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:29.97 +30:46:30.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:29.97 +30:46:30.0: 13.19 +/- 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 10.3316* 02 19 29.97 +30 46 30.0 12.2 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.79 01:44:58.78 +27:48:10.5
137.16161 -33.58506 galactic Psc Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:58.78 +27:48:10.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:44:58.78 +27:48:10.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:44:58.78 +27:48:10.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.79,0.05,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 20260710.3317 12.79CV 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 10.3317 2461231.8317 12.58 02:20:13.49 +30:15:01.8
144.80134 -28.82324 galactic Tri Second-epoch detections are separated by 1.3" and 5.4 pix
The object was found in VSX 1" ASASSN-V J022013.45+301501.7
Type: SR
# Max. Min./Amp. JD0 Period
13.900 V 14.060 V 2456972.00000 142.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:13.49 +30:15:01.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:13.49 +30:15:01.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 13.49 +30 15 01.8 12.6 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022013.45+301501.7,2461231.8317,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022013.45+301501.7 20260710.3317 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.76 01:40:00.84 +28:48:18.7
135.60989 -32.86788 galactic Tri Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:00.84 +28:48:18.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.335+/-0.028 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:40:00.84 +28:48:18.7: 13.63 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:40:00.84 +28:48:18.7: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 01 40 00.84 +28 48 18.7 12.8 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.76CV 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 10.3317 2461231.8317 12.56 02:18:11.85 +31:32:07.8
143.79250 -27.79779 galactic Tri Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:11.85 +31:32:07.8 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:11.85 +31:32:07.8: 13.64 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:11.85 +31:32:07.8: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 18 11.85 +31 32 07.8 12.6 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.54 02:20:39.67 +30:50:14.1
144.64389 -28.24534 galactic Tri Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:39.67 +30:50:14.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.713+/-0.027 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:39.67 +30:50:14.1: 13.48 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:39.67 +30:50:14.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 39.67 +30 50 14.1 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.46 02:19:23.55 +31:18:31.7
144.15589 -27.91252 galactic Tri Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:23.55 +31:18:31.7 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:23.55 +31:18:31.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:23.55 +31:18:31.7: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 19 23.55 +31 18 31.7 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.46,0.05,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 20260710.3317 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.41 02:17:47.34 +29:51:33.5
144.41333 -29.38531 galactic Tri Second-epoch detections are separated by 1.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:17:47.34 +29:51:33.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:47.34 +29:51:33.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:47.34 +29:51:33.5: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 17 47.34 +29 51 33.5 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.44 02:18:37.91 +32:20:11.2
143.55379 -27.01991 galactic Tri Second-epoch detections are separated by 1.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:37.91 +32:20:11.2 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.467+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:37.91 +32:20:11.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:37.91 +32:20:11.2: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 18 37.91 +32 20 11.2 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.46 02:17:42.16 +30:52:56.4
143.95660 -28.44345 galactic Tri Second-epoch detections are separated by 4.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:17:42.16 +30:52:56.4 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:42.16 +30:52:56.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:42.16 +30:52:56.4: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 17 42.16 +30 52 56.4 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.46,0.05,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 20260710.3317 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.46 02:19:01.87 +30:42:28.3
144.33188 -28.49825 galactic Tri Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:01.87 +30:42:28.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.284+/-0.035 (F)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:01.87 +30:42:28.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:01.87 +30:42:28.3: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 19 01.87 +30 42 28.3 12.5 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.46,0.05,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 20260710.3317 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.44 01:48:51.74 +27:53:30.2
138.12865 -33.27979 galactic Tri Second-epoch detections are separated by 1.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 298831218726963456 | 01:48:51.74 +27:53:30.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.473+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:48:51.74 +27:53:30.2: 13.37 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:48:51.74 +27:53:30.2: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 01 48 51.74 +27 53 30.2 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 298831218726963456,2461231.8317,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 298831218726963456 20260710.3317 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.39 02:19:46.50 +31:35:15.5
144.12234 -27.62352 galactic Tri Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.9431+31.5863 | 02:19:44.12 +31:34:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:46.50 +31:35:15.5: 13.34 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:46.50 +31:35:15.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 19 46.50 +31 35 15.5 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J034.9431+31.5863,2461231.8317,12.39,0.05,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
ATO J034.9431+31.5863 20260710.3317 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.06 02:18:01.14 +32:08:08.4
143.50201 -27.25439 galactic Tri Second-epoch detections are separated by 0.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:01.14 +32:08:08.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.394+/-0.035 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:01.14 +32:08:08.4: 13.09 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:01.14 +32:08:08.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 18 01.14 +32 08 08.4 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.06,0.05,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
target 20260710.3317 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.13 01:51:11.41 +28:25:54.3
138.54509 -32.62195 galactic Tri Second-epoch detections are separated by 0.7" and 5.0 pix
The object was found in VSX 1" ASASSN-V J015111.39+282555.2
Type: L
# Max. Min./Amp. JD0 Period
12.830 V 13.120 V
The object was not found in astcheck.
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:51:11.41 +28:25:54.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:51:11.41 +28:25:54.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 01 51 11.41 +28 25 54.3 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015111.39+282555.2,2461231.8317,12.13,0.05,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
ASASSN-V J015111.39+282555.2 20260710.3317 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.38 02:19:36.42 +32:19:52.9
143.77040 -26.94782 galactic Tri Second-epoch detections are separated by 1.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 324923179410615936 | 02:19:36.42 +32:19:52.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:36.42 +32:19:52.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:36.42 +32:19:52.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 19 36.42 +32 19 52.9 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 324923179410615936,2461231.8317,12.38,0.05,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
Large-amplitude variable Gaia DR2 324923179410615936 20260710.3317 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.78 01:59:02.60 +31:40:38.2
139.36859 -29.02754 galactic Tri Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:02.60 +31:40:38.2 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.033 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:59:02.60 +31:40:38.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:59:02.60 +31:40:38.2: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 01 59 02.60 +31 40 38.2 12.8 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.36 02:20:11.16 +29:51:53.9
144.96190 -29.18239 galactic Tri Second-epoch detections are separated by 1.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:11.16 +29:51:53.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.744+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:11.16 +29:51:53.9: 13.31 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:11.16 +29:51:53.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 11.16 +29 51 53.9 12.4 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 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 10.3317 2461231.8317 12.27 02:20:13.75 +31:49:30.7
144.12189 -27.36707 galactic Tri Second-epoch detections are separated by 2.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:13.75 +31:49:30.7 (user input) | T | P | (position from user input) J-Ks=0.768+/-0.027 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:13.75 +31:49:30.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:13.75 +31:49:30.7: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 13.75 +31 49 30.7 12.3 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.64 02:17:07.50 +31:00:38.8
143.77168 -28.37007 galactic Tri Second-epoch detections are separated by 1.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:17:07.50 +31:00:38.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.646+/-0.028 (K)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:07.50 +31:00:38.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:07.50 +31:00:38.8: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 17 07.50 +31 00 38.8 12.6 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.25 02:20:28.59 +32:23:45.1
143.93393 -26.81898 galactic Tri Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:20:28.59 +32:23:45.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.449+/-0.029 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:28.59 +32:23:45.1: 13.25 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:28.59 +32:23:45.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 20 28.59 +32 23 45.1 12.2 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.25,0.05,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 20260710.3317 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3317 2461231.8317 12.28 02:19:26.94 +31:54:33.9
143.91339 -27.35152 galactic Tri Second-epoch detections are separated by 0.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:26.94 +31:54:33.9 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:26.94 +31:54:33.9: 13.25 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:26.94 +31:54:33.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3316* 02 19 26.94 +31 54 33.9 12.3 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8317,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3317 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461231.83189341 10.07.2026 07:57:45.591 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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): 9177
Objects passed selection criteria: 9111
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 5484.5
Average stars matched: 5218.25 (95.1454 %)
Memory usage VmPeak: 115504 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:41:39 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461231.83189341 10.07.2026 07:57:45.591 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 31 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): 57065
Objects passed selection criteria: 56867
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 36155.5
Average stars matched: 34294.8 (94.8535 %)
Memory usage VmPeak: 159652 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:45:19 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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461231.83140830
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
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
Saving wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits to local_wcs_cache/
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
Saving wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits to local_wcs_cache/
'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits'
wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:00:00.720 +29:59:44.33 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:14.660 +29:59:48.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:14.660 +29:59:48.58
Angular distance between the image centers 0.0503 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:14.631 +29:59:18.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:14.631 +29:59:18.44
Angular distance between the image centers 0.0507 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 02:00:14.660 +29:59:48.58
Second-epoch second image center 02:00:14.631 +29:59:18.44
Angular distance between the image centers 0.00837 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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.rlC6B4bz2r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.kLyNzMGSma
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits &> /tmp/tmp.VWlrvY0kAK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits &> /tmp/tmp.LFXmsZS4yr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.6615 deg, Dec +24.4131 to +35.2963 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 20.6045 to 39.6615 deg, Dec 24.4131 to 35.2963 deg
Loaded 8371 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): 6352 out of 6782 total matches.
Matched with Tycho-2 6782 out of 12225 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.922200
a=0.000000 b=1.000000 c=22.922200
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.6615 deg, Dec +24.4131 to +35.2963 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 20.6045 to 39.6615 deg, Dec 24.4131 to 35.2963 deg
Loaded 8371 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): 6352 out of 6782 total matches.
Matched with Tycho-2 6782 out of 12225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=5.9)
Read 12296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.7012 deg, Dec +24.4131 to +35.3109 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 20.6045 to 39.7012 deg, Dec 24.4131 to 35.3109 deg
Loaded 8408 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): 6364 out of 6800 total matches.
Matched with Tycho-2 6800 out of 12296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits (aperture=6.0)
____ 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:
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
2.3 pix fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
2.4 pix fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Limiting magnitude estimates:
15.4 mag. Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.4 mag. Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
12.7 mag. fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
12.6 mag. fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.4 (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.rlC6B4bz2r (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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=932, bad_region=2767, passed=12225
Got 12225 stars (including 8689 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 12225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 9684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 9684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 9683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=958 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.386 n_q1=294 n_q2=210 n_q3=271 n_q4=183 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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.kLyNzMGSma (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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=960, bad_region=2764, passed=12296
Got 12296 stars (including 8751 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 12296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9764 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits N_match=959 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.320 n_q1=291 n_q2=215 n_q3=269 n_q4=184 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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.VWlrvY0kAK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.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=117, bad_region=721, passed=2342
Got 2342 stars (including 1543 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat
util/solve_plate_with_UCAC5 got 2342 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 1696 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 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 1696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 1696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits N_match=952 sigma_overall_arcsec=0.499 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.511 sigma_q3_arcsec=0.543 sigma_q4_arcsec=0.461 n_q1=403 n_q2=189 n_q3=217 n_q4=143 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits -region wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.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.LFXmsZS4yr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.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=93, bad_region=690, passed=2129
Got 2129 stars (including 1381 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat
util/solve_plate_with_UCAC5 got 2129 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 1502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits N_match=949 sigma_overall_arcsec=0.522 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.496 sigma_q3_arcsec=0.626 sigma_q4_arcsec=0.457 n_q1=417 n_q2=207 n_q3=193 n_q4=132 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits -region wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.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=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits sigma_overall=0.349 worst_q_ratio=1.105
ref2=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits sigma_overall=0.302 worst_q_ratio=1.111
new1=fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits sigma_overall=0.499 worst_q_ratio=1.088
new2=fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits sigma_overall=0.522 worst_q_ratio=1.199
reference average sigma_overall=0.3255 worst_q_ratio=1.108
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113_astrometric_residuals.png (958 matched stars from wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114_astrometric_residuals.png (959 matched stars from wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320_astrometric_residuals.png (952 matched stars from wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321_astrometric_residuals.png (949 matched stars from wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits'
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits'
Preparing the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Tri-01-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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Creating symlink local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits exists and is non-empty
wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:00:00.720 +29:59:44.33 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:14.660 +29:59:48.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:14.660 +29:59:48.58
Angular distance between the image centers 0.0503 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:14.631 +29:59:18.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:14.631 +29:59:18.44
Angular distance between the image centers 0.0507 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 02:00:14.660 +29:59:48.58
Second-epoch second image center 02:00:14.631 +29:59:18.44
Angular distance between the image centers 0.00837 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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.J7VB92rIup
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.8fvx9s7GM9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits &> /tmp/tmp.E3lehw3VDp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits &> /tmp/tmp.w50XJQabms
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5720 to 39.6905 deg, Dec +24.3228 to +35.3067 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 20.5720 to 39.6905 deg, Dec 24.3228 to 35.3067 deg
Loaded 8456 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): 5809 out of 6892 total matches.
Matched with Tycho-2 6892 out of 73246 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802700
a=0.000000 b=1.000000 c=22.802700
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5720 to 39.6905 deg, Dec +24.3228 to +35.3067 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 20.5720 to 39.6905 deg, Dec 24.3228 to 35.3067 deg
Loaded 8456 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): 5809 out of 6892 total matches.
Matched with Tycho-2 6892 out of 73246 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=4.6)
Read 72377 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5786 to 39.7012 deg, Dec +24.3308 to +35.3160 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 20.5786 to 39.7012 deg, Dec 24.3308 to 35.3160 deg
Loaded 8467 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): 5844 out of 6896 total matches.
Matched with Tycho-2 6896 out of 72377 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
2.1 pix fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
2.2 pix fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
1.9 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Limiting magnitude estimates:
15.6 mag. Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.6 mag. Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
13.2 mag. fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
13.1 mag. fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.9 (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.J7VB92rIup (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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=14, blended=4778, bad_region=13274, passed=73232
Got 73232 stars (including 55901 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 73232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 61484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 61484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 61485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=953 sigma_overall_arcsec=0.305 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.263 n_q1=287 n_q2=215 n_q3=271 n_q4=180 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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.8fvx9s7GM9 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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=17, blended=4568, bad_region=13126, passed=72360
Got 72360 stars (including 55351 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 72360 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 60809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 60809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 60809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits N_match=952 sigma_overall_arcsec=0.282 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.279 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.277 n_q1=289 n_q2=210 n_q3=275 n_q4=178 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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.E3lehw3VDp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.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=5, blended=466, bad_region=3845, passed=17787
Got 17787 stars (including 13610 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat
util/solve_plate_with_UCAC5 got 17787 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 14297 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 14298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 14298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits N_match=946 sigma_overall_arcsec=0.488 sigma_q1_arcsec=0.463 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.532 sigma_q4_arcsec=0.483 n_q1=397 n_q2=187 n_q3=213 n_q4=149 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits -region wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.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.w50XJQabms (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.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=413, bad_region=3764, passed=16098
Got 16098 stars (including 12067 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat
util/solve_plate_with_UCAC5 got 16098 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits N_match=945 sigma_overall_arcsec=0.510 sigma_q1_arcsec=0.499 sigma_q2_arcsec=0.490 sigma_q3_arcsec=0.595 sigma_q4_arcsec=0.469 n_q1=412 n_q2=209 n_q3=188 n_q4=136 worst_quadrant_to_overall_ratio=1.166
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits -region wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.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_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-03_20.00sec_4.90C_LIGHT_0320.fits
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Tri-01-Q2b1x1_033659_TTUQ2b1x1_1534866_G3UYLiBr/wcs_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321.fits
Preparing the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:55:04.11 +27:16:03.6: 13.56 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:27.27 +27:14:49.7: 11.49 +/- 0.00 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:54.75 +31:16:18.1: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:11:05.77 +30:07:32.7: 12.42 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:40:57.69 +27:09:49.7: 12.17 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:10:15.62 +30:36:55.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:49:52.34 +27:13:36.9: 13.97 +/- 0.05 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:43:40.88 +28:03:09.4: 11.14 +/- 0.00 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:43.76 +32:27:54.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:55:04.11 +27:16:03.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter REJECTED candidate at 01:55:04.11 +27:16:03.6: ref_mag=13.56 +/- 0.03 new_mean_mag=13.0189 delta=0.55 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:52:27.27 +27:14:49.7: 11.44 +/- 0.00 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:40:57.69 +27:09:49.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Forced photometry filter REJECTED candidate at 01:52:27.27 +27:14:49.7: ref_mag=11.46 +/- 0.00 new_mean_mag=11.5422 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:52.39 +32:23:56.6: 13.10 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 01:40:57.69 +27:09:49.7: ref_mag=12.14 +/- 0.01 new_mean_mag=11.9427 delta=0.19 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:43:40.88 +28:03:09.4: 11.09 +/- 0.00 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:49:52.34 +27:13:36.9: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter REJECTED candidate at 01:43:40.88 +28:03:09.4: ref_mag=11.11 +/- 0.00 new_mean_mag=11.0298 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry filter REJECTED candidate at 01:49:52.34 +27:13:36.9: ref_mag=13.93 +/- 0.03 new_mean_mag=13.1357 delta=0.80 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:11:05.77 +30:07:32.7: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 02:11:05.77 +30:07:32.7: ref_mag=12.42 +/- 0.01 new_mean_mag=12.2388 delta=0.18 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:10:15.62 +30:36:55.0: 13.17 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:54.75 +31:16:18.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.01
Forced photometry filter REJECTED candidate at 02:10:15.62 +30:36:55.0: ref_mag=13.16 +/- 0.01 new_mean_mag=12.8325 delta=0.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter REJECTED candidate at 02:17:54.75 +31:16:18.1: ref_mag=13.07 +/- 0.02 new_mean_mag=12.5177 delta=0.56 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:43.76 +32:27:54.6: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 02:18:43.76 +32:27:54.6: ref_mag=13.36 +/- 0.02 new_mean_mag=12.4122 delta=0.95 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:52.39 +32:23:56.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.01
Forced photometry filter KEPT candidate at 02:18:52.39 +32:23:56.6: ref_mag=13.11 +/- 0.01 new_mean_mag=12.1928 delta=0.92 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:37.66 +30:22:24.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:54.45 +31:58:37.3: 12.94 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:54.79 +31:08:26.2: 13.21 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:51:19.97 +28:28:38.1: 13.88 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:29.97 +30:46:30.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:25.93 +31:06:18.0: 13.23 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:37.66 +30:22:24.6: 13.52 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:54.45 +31:58:37.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:37.66 +30:22:24.6: ref_mag=13.49 +/- 0.02 new_mean_mag=12.5121 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.96 +/- 0.01
Forced photometry filter KEPT candidate at 02:20:54.45 +31:58:37.3: ref_mag=12.96 +/- 0.01 new_mean_mag=12.0448 delta=0.92 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:54.79 +31:08:26.2: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 02:20:54.79 +31:08:26.2: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2375 delta=0.98 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:44:58.78 +27:48:10.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:29.97 +30:46:30.0: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:29.97 +30:46:30.0: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1928 delta=1.00 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:51:19.97 +28:28:38.1: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Forced photometry filter KEPT candidate at 01:51:19.97 +28:28:38.1: ref_mag=13.90 +/- 0.03 new_mean_mag=12.8624 delta=1.04 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:25.93 +31:06:18.0: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:25.93 +31:06:18.0: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1517 delta=1.07 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:44:58.78 +27:48:10.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 01:44:58.78 +27:48:10.5: ref_mag=13.73 +/- 0.03 new_mean_mag=12.7893 delta=0.94 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:39:19.89 +29:28:40.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:39:19.89 +29:28:40.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 01:39:19.89 +29:28:40.1: ref_mag=13.67 +/- 0.04 new_mean_mag=12.6950 delta=0.98 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:13.49 +30:15:01.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:13.49 +30:15:01.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 02:20:13.49 +30:15:01.8: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5735 delta=1.11 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:40:00.84 +28:48:18.7: 13.63 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:40:00.84 +28:48:18.7: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 01:40:00.84 +28:48:18.7: ref_mag=13.65 +/- 0.03 new_mean_mag=12.7109 delta=0.94 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:11.85 +31:32:07.8: 13.64 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:11.85 +31:32:07.8: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 02:18:11.85 +31:32:07.8: ref_mag=13.64 +/- 0.02 new_mean_mag=12.5276 delta=1.11 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:39.67 +30:50:14.1: 13.48 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:39.67 +30:50:14.1: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 02:20:39.67 +30:50:14.1: ref_mag=13.52 +/- 0.02 new_mean_mag=12.5412 delta=0.98 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:23.55 +31:18:31.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:47.34 +29:51:33.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:23.55 +31:18:31.7: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:47.34 +29:51:33.5: 13.43 +/- 0.03 detection
Forced photometry filter KEPT candidate at 02:19:23.55 +31:18:31.7: ref_mag=13.47 +/- 0.02 new_mean_mag=12.4395 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 02:17:47.34 +29:51:33.5: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4093 delta=1.01 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:37.91 +32:20:11.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:42.16 +30:52:56.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:37.91 +32:20:11.2: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 02:18:37.91 +32:20:11.2: ref_mag=13.36 +/- 0.02 new_mean_mag=12.4341 delta=0.93 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:42.16 +30:52:56.4: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 02:17:42.16 +30:52:56.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4612 delta=0.91 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:01.87 +30:42:28.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:48:51.74 +27:53:30.2: 13.37 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:01.87 +30:42:28.3: 13.40 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:46.50 +31:35:15.5: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:01.87 +30:42:28.3: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4569 delta=0.94 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:48:51.74 +27:53:30.2: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 01:48:51.74 +27:53:30.2: ref_mag=13.35 +/- 0.02 new_mean_mag=12.4336 delta=0.91 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:46.50 +31:35:15.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:46.50 +31:35:15.5: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3941 delta=0.91 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:18:01.14 +32:08:08.4: 13.09 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:18:01.14 +32:08:08.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 02:18:01.14 +32:08:08.4: ref_mag=13.08 +/- 0.01 new_mean_mag=12.0597 delta=1.02 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:51:11.41 +28:25:54.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:51:11.41 +28:25:54.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 01:51:11.41 +28:25:54.3: ref_mag=13.02 +/- 0.01 new_mean_mag=12.0943 delta=0.93 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:36.42 +32:19:52.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:36.42 +32:19:52.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:36.42 +32:19:52.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3814 delta=0.98 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:59:02.60 +31:40:38.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:11.16 +29:51:53.9: 13.31 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:13.75 +31:49:30.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:59:02.60 +31:40:38.2: 13.81 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:11.16 +29:51:53.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 01:59:02.60 +31:40:38.2: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7325 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 02:20:11.16 +29:51:53.9: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3510 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:13.75 +31:49:30.7: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 02:20:13.75 +31:49:30.7: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2608 delta=1.00 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:07.50 +31:00:38.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:28.59 +32:23:45.1: 13.25 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:07.50 +31:00:38.8: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 02:17:07.50 +31:00:38.8: ref_mag=13.74 +/- 0.03 new_mean_mag=12.6031 delta=1.13 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:28.59 +32:23:45.1: 13.21 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:26.94 +31:54:33.9: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 02:20:28.59 +32:23:45.1: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2576 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:26.94 +31:54:33.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 02:19:26.94 +31:54:33.9: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2880 delta=1.00 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out45142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72358.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 55s
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: 20s
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Considering the candidate 87325_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 87325_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 87330_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 87330_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 87331_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 87331_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 87332_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 87332_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 88407_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 88407_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
**** FOUND 01:53:01.17 +29:36:55.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 89048_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 89048_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 89810_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 89810_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 89967_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 89967_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 90269_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 90269_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
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Considering the candidate 21059_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 21059_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 21513_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 21513_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 37103_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 37103_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 24602_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 24602_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 72358_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 72358_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 31487_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 31487_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 31070_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 31070_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 34041_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 34041_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 67038_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 67038_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 70911_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 70911_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
**** FOUND 02:19:29.18 +28:04:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45142_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 45142_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
**** FOUND 01:39:19.89 +29:28:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.314 302265749455132928 024.83286662903 +29.47789237241 13.4461 12.9562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 37966_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 37966_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 62713_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 62713_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
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Considering the candidate 28433_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 28433_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33462_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 33462_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29971_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 29971_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41139_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 41139_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22022_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 22022_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33439_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 33439_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34581_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 34581_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67710_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 67710_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27794_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 27794_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23608_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 23608_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72030_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 72030_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21983_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 21983_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28697_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 28697_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40843_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 40843_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25900_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 25900_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32503_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 32503_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21357_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 21357_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25355_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
Preparing report for the candidate 25355_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68673_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321
The candidate 68673_fd_Tri-01-Q2b1x1_2026-07-10_02-57-45_20.00sec_5.00C_LIGHT_0321 did not pass the final checks
**** FOUND 02:07:50.84 +27:56:14.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 78s
Prepared the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:18:43.76 +32:27:54.6
02:20:28.59 +32:23:45.1
02:18:52.39 +32:23:56.6
02:19:36.42 +32:19:52.9
02:18:37.91 +32:20:11.2
02:18:01.14 +32:08:08.4
02:20:54.45 +31:58:37.3
02:19:26.94 +31:54:33.9
02:20:13.75 +31:49:30.7
02:19:46.50 +31:35:15.5
02:18:11.85 +31:32:07.8
01:59:02.60 +31:40:38.2
02:19:23.55 +31:18:31.7
02:20:54.79 +31:08:26.2
02:19:25.93 +31:06:18.0
02:17:07.50 +31:00:38.8
02:17:42.16 +30:52:56.4
02:20:39.67 +30:50:14.1
02:19:29.97 +30:46:30.0
02:19:01.87 +30:42:28.3
02:19:37.66 +30:22:24.6
02:20:13.49 +30:15:01.8
02:20:11.16 +29:51:53.9
02:17:47.34 +29:51:33.5
01:40:00.84 +28:48:18.7
01:44:58.78 +27:48:10.5
01:48:51.74 +27:53:30.2
01:51:11.41 +28:25:54.3
01:51:19.97 +28:28:38.1
########### Completed Tri-01-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 ####
02:18:43.76 +32:27:54.6
02:18:52.39 +32:23:56.6
02:19:37.66 +30:22:24.6
02:20:54.45 +31:58:37.3
01:51:19.97 +28:28:38.1
02:19:25.93 +31:06:18.0
02:20:54.79 +31:08:26.2
02:19:29.97 +30:46:30.0
01:44:58.78 +27:48:10.5
02:20:13.49 +30:15:01.8
01:40:00.84 +28:48:18.7
02:18:11.85 +31:32:07.8
02:20:39.67 +30:50:14.1
02:19:23.55 +31:18:31.7
02:17:47.34 +29:51:33.5
02:18:37.91 +32:20:11.2
02:17:42.16 +30:52:56.4
02:19:01.87 +30:42:28.3
01:48:51.74 +27:53:30.2
02:19:46.50 +31:35:15.5
02:18:01.14 +32:08:08.4
01:51:11.41 +28:25:54.3
02:19:36.42 +32:19:52.9
01:59:02.60 +31:40:38.2
02:20:11.16 +29:51:53.9
02:20:13.75 +31:49:30.7
02:17:07.50 +31:00:38.8
02:20:28.59 +32:23:45.1
02:19:26.94 +31:54:33.9
###################################################################################
02:18:43.76 +32:27:54.6 -- not an asteroid (will add it to exclusion list)
02:18:52.39 +32:23:56.6 -- not an asteroid (will add it to exclusion list)
02:19:37.66 +30:22:24.6 -- not an asteroid (will add it to exclusion list)
02:20:54.45 +31:58:37.3 -- not an asteroid (will add it to exclusion list)
01:51:19.97 +28:28:38.1 -- not an asteroid (will add it to exclusion list)
02:19:25.93 +31:06:18.0 -- not an asteroid (will add it to exclusion list)
02:20:54.79 +31:08:26.2 -- not an asteroid (will add it to exclusion list)
02:19:29.97 +30:46:30.0 -- not an asteroid (will add it to exclusion list)
01:44:58.78 +27:48:10.5 -- not an asteroid (will add it to exclusion list)
02:20:13.49 +30:15:01.8 -- not an asteroid (will add it to exclusion list)
01:40:00.84 +28:48:18.7 -- not an asteroid (will add it to exclusion list)
02:18:11.85 +31:32:07.8 -- not an asteroid (will add it to exclusion list)
02:20:39.67 +30:50:14.1 -- not an asteroid (will add it to exclusion list)
02:19:23.55 +31:18:31.7 -- not an asteroid (will add it to exclusion list)
02:17:47.34 +29:51:33.5 -- not an asteroid (will add it to exclusion list)
02:18:37.91 +32:20:11.2 -- not an asteroid (will add it to exclusion list)
02:17:42.16 +30:52:56.4 -- not an asteroid (will add it to exclusion list)
02:19:01.87 +30:42:28.3 -- not an asteroid (will add it to exclusion list)
01:48:51.74 +27:53:30.2 -- not an asteroid (will add it to exclusion list)
02:19:46.50 +31:35:15.5 -- not an asteroid (will add it to exclusion list)
02:18:01.14 +32:08:08.4 -- not an asteroid (will add it to exclusion list)
01:51:11.41 +28:25:54.3 -- not an asteroid (will add it to exclusion list)
02:19:36.42 +32:19:52.9 -- not an asteroid (will add it to exclusion list)
01:59:02.60 +31:40:38.2 -- not an asteroid (will add it to exclusion list)
02:20:11.16 +29:51:53.9 -- not an asteroid (will add it to exclusion list)
02:20:13.75 +31:49:30.7 -- not an asteroid (will add it to exclusion list)
02:17:07.50 +31:00:38.8 -- not an asteroid (will add it to exclusion list)
02:20:28.59 +32:23:45.1 -- not an asteroid (will add it to exclusion list)
02:19:26.94 +31:54:33.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:40:00.84 +28:48:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:58.78 +27:48:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:51.74 +27:53:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:11.41 +28:25:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:19.97 +28:28:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:02.60 +31:40:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:07.50 +31:00:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:42.16 +30:52:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:47.34 +29:51:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:01.14 +32:08:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:11.85 +31:32:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:37.91 +32:20:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:43.76 +32:27:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:52.39 +32:23:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:01.87 +30:42:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:23.55 +31:18:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:25.93 +31:06:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:26.94 +31:54:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:29.97 +30:46:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.42 +32:19:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:37.66 +30:22:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:46.50 +31:35:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:11.16 +29:51:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:13.49 +30:15:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:13.75 +31:49:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:28.59 +32:23:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:39.67 +30:50:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.45 +31:58:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.79 +31:08:26.2 -- 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)
01:40:00.84 +28:48:18.7 -- not a known variable star
01:44:58.78 +27:48:10.5 -- not a known variable star
01:48:51.74 +27:53:30.2 -- not a known variable star
01:51:11.41 +28:25:54.3 -- a known variable star
01:51:19.97 +28:28:38.1 -- not a known variable star
01:59:02.60 +31:40:38.2 -- not a known variable star
02:17:07.50 +31:00:38.8 -- not a known variable star
02:17:42.16 +30:52:56.4 -- not a known variable star
02:17:47.34 +29:51:33.5 -- not a known variable star
02:18:01.14 +32:08:08.4 -- not a known variable star
02:18:11.85 +31:32:07.8 -- not a known variable star
02:18:37.91 +32:20:11.2 -- not a known variable star
02:18:43.76 +32:27:54.6 -- not a known variable star
02:18:52.39 +32:23:56.6 -- not a known variable star
02:19:01.87 +30:42:28.3 -- not a known variable star
02:19:23.55 +31:18:31.7 -- not a known variable star
02:19:25.93 +31:06:18.0 -- not a known variable star
02:19:26.94 +31:54:33.9 -- not a known variable star
02:19:29.97 +30:46:30.0 -- not a known variable star
02:19:36.42 +32:19:52.9 -- not a known variable star
02:19:37.66 +30:22:24.6 -- not a known variable star
02:19:46.50 +31:35:15.5 -- not a known variable star
02:20:11.16 +29:51:53.9 -- not a known variable star
02:20:13.49 +30:15:01.8 -- a known variable star
02:20:13.75 +31:49:30.7 -- not a known variable star
02:20:28.59 +32:23:45.1 -- not a known variable star
02:20:39.67 +30:50:14.1 -- not a known variable star
02:20:54.45 +31:58:37.3 -- not a known variable star
02:20:54.79 +31:08:26.2 -- not a known variable star
Found 27 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
29 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
01:40:00.84 +28:48:18.7
01:44:58.78 +27:48:10.5
01:48:51.74 +27:53:30.2
01:51:11.41 +28:25:54.3
01:51:19.97 +28:28:38.1
01:59:02.60 +31:40:38.2
02:17:07.50 +31:00:38.8
02:17:42.16 +30:52:56.4
02:17:47.34 +29:51:33.5
02:18:01.14 +32:08:08.4
02:18:11.85 +31:32:07.8
02:18:37.91 +32:20:11.2
02:18:43.76 +32:27:54.6
02:18:52.39 +32:23:56.6
02:19:01.87 +30:42:28.3
02:19:23.55 +31:18:31.7
02:19:25.93 +31:06:18.0
02:19:26.94 +31:54:33.9
02:19:29.97 +30:46:30.0
02:19:36.42 +32:19:52.9
02:19:37.66 +30:22:24.6
02:19:46.50 +31:35:15.5
02:20:11.16 +29:51:53.9
02:20:13.49 +30:15:01.8
02:20:13.75 +31:49:30.7
02:20:28.59 +32:23:45.1
02:20:39.67 +30:50:14.1
02:20:54.45 +31:58:37.3
02:20:54.79 +31:08:26.2
01:39:19.89 +29:28:40.1
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461231.83140830 -observatory V36
07:32:19.70 +17:08:04.0 Mercury (5.1mag)
10:11:33.89 +12:41:30.1 Venus (-4.1mag)
04:24:06.90 +21:25:03.5 Mars (1.3mag)
08:16:39.51 +20:11:32.3 Jupiter (-1.8mag)
00:55:50.78 +03:20:28.4 Saturn (0.7mag)
04:07:13.81 +20:45:02.8 Uranus (5.8mag)
00:17:01.50 +00:20:41.3 Neptune (7.8mag)
20:30:55.05 -23:18:00.1 Pluto (14.4mag)
03:10:31.08 +22:13:54.5 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 03:41 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.83140830:
08:16:45.98 +20:11:09.9 Io (6.1mag)
08:16:42.03 +20:11:24.7 Europa (6.3mag)
08:16:56.52 +20:10:30.9 Ganymede (5.6mag)
08:17:07.56 +20:09:48.7 Callisto (6.8mag)
08:15:11.05 +19:55:41.4 Himalia (15.7mag)
08:16:38.33 +20:11:37.7 Thebe (16.6mag)
08:14:32.40 +20:00:11.2 Elara (17.6mag)
08:20:11.69 +20:05:43.0 Pasiphae (17.8mag)
08:21:37.42 +20:16:37.1 Carme (19.0mag)
00:55:40.60 +03:20:19.4 Titan (8.5mag)
00:55:45.54 +03:20:31.7 Rhea (9.8mag)
00:55:20.10 +03:19:37.5 Iapetus (11.2mag)
00:56:00.09 +03:20:47.3 Hyperion (14.5mag)
00:55:51.53 +03:17:42.3 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 03:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.83140830:
17:46:10.50 -32:59:57.8 JWST
16:12:05.26 +49:11:16.1 Chandra
01:57:24.18 +63:42:12.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 03:41 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.83140830 -observatory V36
02:36:14.45 +14:25:33.0 17.9mag P/1996 R2 (Lagerkvist)
18:17:57.33 -34:21:43.5 13.7mag P/2010 H2 (Vales)
06:25:39.26 -68:08:21.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:47.94 +32:26:47.8 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.31 +16:02:54.9 18.0mag C/2021 G2 (ATLAS)
01:47:41.40 +08:10:48.4 15.4mag P/2021 N1 (ZTF)
22:59:32.61 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:22.57 +26:55:35.3 16.7mag C/2022 N2 (PANSTARRS)
09:55:29.84 +29:46:54.5 16.8mag C/2022 QE78 (ATLAS)
09:09:43.32 +04:59:55.7 17.8mag C/2022 R6 (PANSTARRS)
18:07:13.83 +21:17:40.7 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.36 -11:23:14.4 17.7mag P/2023 B1 (PANSTARRS)
21:49:15.56 +67:37:17.0 17.8mag C/2023 H5 (Lemmon)
16:30:55.56 -10:04:34.0 13.9mag C/2023 R1 (PANSTARRS)
08:00:36.90 +65:42:26.4 17.9mag C/2024 A1 (ATLAS)
07:32:47.25 +30:00:08.2 14.6mag C/2024 E1 (Wierzchos)
15:16:20.17 +15:19:40.1 17.5mag C/2024 G6 (ATLAS)
19:41:20.14 +39:23:20.5 13.8mag C/2024 J3 (ATLAS)
21:47:36.23 +46:00:00.6 17.8mag C/2024 R4 (PANSTARRS)
04:49:37.19 -13:47:48.6 15.7mag C/2024 T5 (ATLAS)
06:34:33.36 +29:04:23.7 18.0mag C/2025 J1 (Borisov)
07:14:19.47 -12:53:16.3 16.5mag C/2025 R3 (PANSTARRS)
09:56:04.08 +22:26:15.8 17.6mag C/2025 V2 (Rankin)
12:44:36.61 +03:56:19.2 17.1mag C/2025 Y1 (ATLAS)
16:52:00.75 +79:07:11.7 17.4mag C/2026 A2 (Bok)
02:46:15.23 +45:14:20.0 16.7mag C/2026 B2 (Sun-Gao)
11:25:29.88 +04:32:25.6 16.9mag A/2026 E1
21:19:00.37 -15:04:09.0 7.3mag 10P/Tempel
11:13:26.72 -01:53:10.8 16.1mag 29P/Schwassmann-Wachmann
04:00:08.54 +29:33:03.2 17.8mag 47P/Ashbrook-Jackson
10:08:01.97 +14:01:04.9 17.0mag 63P/Wild
00:48:21.20 -05:05:36.2 15.5mag 65P/Gunn
08:26:53.27 +34:13:11.3 17.9mag 76P/West-Kohoutek-Ikemura
04:27:20.86 +20:10:39.5 13.7mag 78P/Gehrels
02:22:18.02 +10:36:23.7 16.2mag 88P/Howell
06:35:28.08 +30:32:09.4 15.7mag 93P/Lovas
04:20:55.90 +31:07:19.3 16.9mag 114P/Wiseman-Skiff
08:08:38.59 +30:42:20.9 15.3mag 123P/West-Hartley
10:48:05.53 +01:11:43.5 16.8mag 124P/Mrkos
04:51:41.67 +20:48:44.4 16.2mag 128P/Shoemaker-Holt
05:36:12.95 +19:42:51.0 17.8mag 131P/Mueller
00:01:32.38 +02:56:03.9 17.9mag 139P/Vaisala-Oterma
07:13:29.04 +17:01:30.7 15.5mag 141P-D/Machholz
03:16:50.40 -21:06:27.5 15.5mag 161P/Hartley-IRAS
05:32:59.28 +33:56:38.4 15.3mag 162P/SidingSpring
19:04:31.61 +15:04:11.8 14.7mag 169P/NEAT
01:40:58.82 +07:35:46.5 17.7mag 220P/McNaught
16:35:58.33 -08:23:04.5 17.0mag 235P/LINEAR
08:45:14.47 +33:18:04.9 17.9mag 240P/NEAT
20:42:11.09 -49:33:57.5 17.8mag 259P/Garradd
01:59:14.88 +12:05:05.9 15.7mag 260P/McNaught
05:37:09.75 +36:50:28.2 17.4mag 295P/LINEAR
15:06:36.87 +06:03:31.5 17.6mag 391P/Kowalski
08:34:35.08 +19:40:39.4 17.9mag 450P/LONEOS
07:51:44.01 +39:13:04.4 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 03:41 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 10 03:41 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 03:41 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
-rw-r--r-- 1 apache apache 30K Jul 10 03:41 tns_transients_list.txt
