This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8
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 08 07.1224 2461259.6224 9.66 18:38:27.27 -12:55:37.7
19.95380 -3.03205 galactic Sct Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.18 Melpomene -0 -0 0 9.3 -0 0
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:38:27.27 -12:55:37.7: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:38:27.27 -12:55:37.7: 15.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
VARIABLE_NAME,2461259.6224,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260807.1224 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 8.99 19:10:55.24 -13:16:13.6
23.18346 -10.26601 galactic Sgr Second-epoch detections are separated by 0.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.7307-13.2616 | 19:10:55.28 -13:16:13.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.728+/-0.037 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:55.24 -13:16:13.6: 9.96 +/- 0.00 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:55.24 -13:16:13.6: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.7307-13.2616,2461259.6224,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7307-13.2616 20260807.1224 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.03 19:10:06.87 -13:20:30.1
23.03183 -10.12016 galactic Sgr Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.5287-13.3415 | 19:10:06.90 -13:20:29.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.794+/-0.029 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:06.87 -13:20:30.1: 12.17 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:06.87 -13:20:30.1: 12.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.5287-13.3415,2461259.6224,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.5287-13.3415 20260807.1224 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.40 19:07:40.65 -13:30:22.0
22.62027 -9.65775 galactic Sgr Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197486965906621824 | 19:07:39.81 -13:30:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.756+/-0.031 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:07:40.65 -13:30:22.0: 12.42 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:07:40.65 -13:30:22.0: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197486965906621824,2461259.6224,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197486965906621824 20260807.1224 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.51 19:11:01.82 -13:27:52.0
23.01747 -10.37408 galactic Sgr Second-epoch detections are separated by 2.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:11:01.82 -13:27:52.0 (user input) | T | P | (position from user input) J-Ks=0.745+/-0.031 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:01.82 -13:27:52.0: 12.78 +/- 0.05 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:01.82 -13:27:52.0: 13.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461259.6224,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260807.1224 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.41 19:11:04.10 -13:31:59.8
22.95844 -10.41219 galactic Sgr Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197511017725788288 | 19:11:04.09 -13:32:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.253+/-0.033 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:04.10 -13:31:59.8: 12.47 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:04.10 -13:31:59.8: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197511017725788288,2461259.6224,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197511017725788288 20260807.1224 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.45 19:09:22.31 -13:22:23.1
22.92351 -9.97103 galactic Sgr Second-epoch detections are separated by 3.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.3490-13.3733 | 19:09:22.28 -13:22:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.804+/-0.033 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:22.31 -13:22:23.1: 12.47 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:22.31 -13:22:23.1: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.3490-13.3733,2461259.6224,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.3490-13.3733 20260807.1224 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.32 19:10:46.50 -13:16:03.6
23.17039 -10.23287 galactic Sgr Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197553383277620352 | 19:10:46.55 -13:16:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.720+/-0.031 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:46.50 -13:16:03.6: 12.44 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:46.50 -13:16:03.6: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.54 +/- 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
Gaia DR3 4197553383277620352,2461259.6224,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197553383277620352 20260807.1224 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.40 19:11:18.16 -13:35:09.7
22.93513 -10.48636 galactic Sgr Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.8202-13.5939 | 19:11:16.85 -13:35:38.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.029 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:18.16 -13:35:09.7: 12.43 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:18.16 -13:35:09.7: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.8202-13.5939,2461259.6224,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.8202-13.5939 20260807.1224 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.43 19:09:37.66 -13:15:13.4
23.06012 -9.97528 galactic Sgr Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.4118-13.2531 | 19:09:37.67 -13:15:13.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.030 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:37.66 -13:15:13.4: 12.42 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:37.66 -13:15:13.4: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.4118-13.2531,2461259.6224,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.4118-13.2531 20260807.1224 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.33 19:09:22.95 -13:12:30.4
23.07521 -9.90187 galactic Sgr Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.3477-13.2008 | 19:09:22.91 -13:12:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.035 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:22.95 -13:12:30.4: 12.39 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:22.95 -13:12:30.4: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.3477-13.2008,2461259.6224,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.3477-13.2008 20260807.1224 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.13 19:10:57.74 -13:14:24.9
23.21558 -10.26206 galactic Sgr Second-epoch detections are separated by 1.9" 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 | Gaia DR3 4197553559395010432 | 19:10:55.34 -13:14:42.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.281+/-0.035 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:57.74 -13:14:24.9: 12.34 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:57.74 -13:14:24.9: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.44 +/- 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
Gaia DR3 4197553559395010432,2461259.6224,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197553559395010432 20260807.1224 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.28 19:08:55.89 -13:42:34.7
22.56845 -10.02060 galactic Sgr Second-epoch detections are separated by 1.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197420071814339584 | 19:08:55.91 -13:42:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.822+/-0.030 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:55.89 -13:42:34.7: 12.32 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:55.89 -13:42:34.7: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197420071814339584,2461259.6224,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197420071814339584 20260807.1224 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.29 19:08:13.22 -13:14:51.2
22.91468 -9.66417 galactic Sgr Second-epoch detections are separated by 1.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197590152517588224 | 19:08:12.68 -13:14:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.144+/-0.035 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:13.22 -13:14:51.2: 12.27 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:13.22 -13:14:51.2: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197590152517588224,2461259.6224,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197590152517588224 20260807.1224 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.28 19:09:06.44 -13:21:22.7
22.91049 -9.90579 galactic Sgr Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.2768-13.3565 | 19:09:06.44 -13:21:23.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.281+/-0.030 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:06.44 -13:21:22.7: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:06.44 -13:21:22.7: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.2768-13.3565,2461259.6224,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.2768-13.3565 20260807.1224 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.27 19:09:42.89 -13:47:11.3
22.58181 -10.22533 galactic Sgr Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197406289240949632 | 19:09:42.97 -13:47:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.683+/-0.032 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:42.89 -13:47:11.3: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:42.89 -13:47:11.3: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197406289240949632,2461259.6224,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197406289240949632 20260807.1224 11.27CV 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 08 07.1224 2461259.6224 11.18 19:09:11.85 -13:40:26.6
22.62946 -10.06340 galactic Sgr Second-epoch detections are separated by 3.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.2962-13.6722 | 19:09:11.93 -13:40:27.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.001+/-0.033 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:11.85 -13:40:26.6: 12.20 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:11.85 -13:40:26.6: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.2962-13.6722,2461259.6224,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.2962-13.6722 20260807.1224 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.24 19:11:08.40 -13:27:27.4
23.03546 -10.39516 galactic Sgr Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197512014158197888 | 19:11:08.37 -13:27:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.780+/-0.030 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:08.40 -13:27:27.4: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:08.40 -13:27:27.4: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197512014158197888,2461259.6224,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197512014158197888 20260807.1224 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.21 19:08:39.31 -13:13:01.3
22.98927 -9.74618 galactic Sgr Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1600-13.2233 | 19:08:39.27 -13:13:01.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.408+/-0.033 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:39.31 -13:13:01.3: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:39.31 -13:13:01.3: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.1600-13.2233,2461259.6224,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1600-13.2233 20260807.1224 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.32 19:11:21.18 -13:57:12.8
22.60328 -10.65610 galactic Sgr Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4185469101960379776 | 19:11:21.17 -13:57:13.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.871+/-0.036 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:21.18 -13:57:12.8: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:21.18 -13:57:12.8: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4185469101960379776,2461259.6224,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4185469101960379776 20260807.1224 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.13 19:10:26.78 -13:27:24.7
22.96192 -10.24281 galactic Sgr Second-epoch detections are separated by 0.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197523009274475520 | 19:10:26.82 -13:27:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.769+/-0.033 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:26.78 -13:27:24.7: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:26.78 -13:27:24.7: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197523009274475520,2461259.6224,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197523009274475520 20260807.1224 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.05 19:08:33.16 -13:17:20.5
22.91248 -9.75503 galactic Sgr Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197585853230369152 | 19:08:32.88 -13:17:20.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:33.16 -13:17:20.5: 12.13 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:33.16 -13:17:20.5: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197585853230369152,2461259.6224,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197585853230369152 20260807.1224 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.09 19:09:28.49 -13:16:08.4
23.02975 -9.94841 galactic Sgr Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197579741516496768 | 19:09:28.51 -13:16:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.033 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:28.49 -13:16:08.4: 12.09 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:28.49 -13:16:08.4: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197579741516496768,2461259.6224,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197579741516496768 20260807.1224 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.20 19:11:05.88 -14:31:54.2
22.04506 -10.84931 galactic Sgr Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.7720-14.5355 | 19:11:05.89 -14:31:54.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.185+/-0.033 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:05.88 -14:31:54.2: 12.10 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:05.88 -14:31:54.2: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.7720-14.5355,2461259.6224,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7720-14.5355 20260807.1224 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.08 19:09:35.28 -13:30:58.1
22.81577 -10.08045 galactic Sgr Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197520088696716544 | 19:09:35.26 -13:30:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.621+/-0.030 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:35.28 -13:30:58.1: 12.09 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:35.28 -13:30:58.1: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197520088696716544,2461259.6224,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197520088696716544 20260807.1224 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 11.04 19:10:30.55 -13:16:09.0
23.14052 -10.17523 galactic Sgr Second-epoch detections are separated by 1.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197553898673696128 | 19:10:30.49 -13:16:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.786+/-0.032 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:30.55 -13:16:09.0: 12.03 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:30.55 -13:16:09.0: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197553898673696128,2461259.6224,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197553898673696128 20260807.1224 11.04CV 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 08 07.1224 2461259.6224 11.04 19:10:06.81 -13:29:34.4
22.89331 -10.18549 galactic Sgr Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197523146713430656 | 19:10:06.78 -13:29:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.161+/-0.032 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:06.81 -13:29:34.4: 11.93 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:06.81 -13:29:34.4: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197523146713430656,2461259.6224,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197523146713430656 20260807.1224 11.04CV 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 08 07.1224 2461259.6224 11.05 19:08:40.09 -13:52:20.0
22.39152 -10.03345 galactic Sgr Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197410652927712512 | 19:08:40.09 -13:52:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.730+/-0.032 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:40.09 -13:52:20.0: 11.90 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:40.09 -13:52:20.0: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197410652927712512,2461259.6224,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197410652927712512 20260807.1224 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.97 19:08:08.91 -13:21:07.0
22.81162 -9.69385 galactic Sgr Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.0360-13.3471 | 19:08:08.98 -13:21:06.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.602+/-0.032 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:08.91 -13:21:07.0: 11.89 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:08.91 -13:21:07.0: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.0360-13.3471,2461259.6224,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0360-13.3471 20260807.1224 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.96 19:08:44.36 -13:20:30.4
22.88430 -9.81885 galactic Sgr Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.1816-13.3440 | 19:08:44.36 -13:20:31.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.138+/-0.037 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:44.36 -13:20:30.4: 11.85 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:44.36 -13:20:30.4: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.1816-13.3440,2461259.6224,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1816-13.3440 20260807.1224 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.73 19:08:58.41 -13:18:06.1
22.94607 -9.85274 galactic Sgr Second-epoch detections are separated by 0.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197574239638811904 | 19:08:58.42 -13:18:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.001+/-0.043 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:58.41 -13:18:06.1: 11.82 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:58.41 -13:18:06.1: 11.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197574239638811904,2461259.6224,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197574239638811904 20260807.1224 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.94 19:09:59.67 -13:14:39.9
23.10798 -10.05165 galactic Sgr Second-epoch detections are separated by 1.3" and 6.1 pix
The object was found in VSX 2" ASASSN-V J190959.78-131438.8
Type: SR
# Max. Min./Amp. JD0 Period
13.240 g Y 0.290 g 2458392.67100 30.790000000000
The object was not found in astcheck.
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:59.67 -13:14:39.9: 11.81 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:59.67 -13:14:39.9: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190959.78-131438.8,2461259.6224,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190959.78-131438.8 20260807.1224 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.75 19:09:20.17 -13:15:42.9
23.02135 -9.91494 galactic Sgr Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197579982034709760 | 19:09:20.12 -13:15:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.204+/-0.033 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:20.17 -13:15:42.9: 11.75 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:20.17 -13:15:42.9: 11.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197579982034709760,2461259.6224,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197579982034709760 20260807.1224 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.72 19:10:08.60 -13:25:53.9
22.95258 -10.16548 galactic Sgr Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197526930596929152 | 19:10:08.57 -13:25:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.183+/-0.037 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:08.60 -13:25:53.9: 11.64 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:08.60 -13:25:53.9: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197526930596929152,2461259.6224,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197526930596929152 20260807.1224 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.64 19:10:55.31 -13:14:41.0
23.20714 -10.25512 galactic Sgr Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197553559395010432 | 19:10:55.34 -13:14:42.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.057+/-0.033 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:55.31 -13:14:41.0: 11.65 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:55.31 -13:14:41.0: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197553559395010432,2461259.6224,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197553559395010432 20260807.1224 10.64CV 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 08 07.1224 2461259.6224 10.63 19:10:49.28 -13:21:25.2
23.09354 -10.28174 galactic Sgr Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.7172-13.3522 | 19:10:49.18 -13:21:25.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.033 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:49.28 -13:21:25.2: 11.60 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:49.28 -13:21:25.2: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.7172-13.3522,2461259.6224,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7172-13.3522 20260807.1224 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.59 19:10:35.49 -13:30:22.3
22.93227 -10.29599 galactic Sgr Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.6571-13.5065 | 19:10:35.46 -13:30:22.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.030 (G)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:35.49 -13:30:22.3: 11.50 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:35.49 -13:30:22.3: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.6571-13.5065,2461259.6224,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.6571-13.5065 20260807.1224 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.53 19:09:21.36 -13:19:46.7
22.96155 -9.94870 galactic Sgr Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.3451-13.3276 | 19:09:21.31 -13:19:46.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.035 (F)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:21.36 -13:19:46.7: 11.50 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:21.36 -13:19:46.7: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.3451-13.3276,2461259.6224,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.3451-13.3276 20260807.1224 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.35 19:11:04.99 -13:22:06.4
23.11109 -10.34410 galactic Sgr Second-epoch detections are separated by 1.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197548504200340096 | 19:11:04.99 -13:22:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.773+/-0.053 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:04.99 -13:22:06.4: 11.26 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:04.99 -13:22:06.4: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197548504200340096,2461259.6224,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197548504200340096 20260807.1224 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.00 19:11:11.46 -13:15:48.6
23.21879 -10.32229 galactic Sgr Second-epoch detections are separated by 1.1" and 5.8 pix
The object was found in VSX12" ZTF J191112.08-131555.9
Type: RS
# Max. Min./Amp. JD0 Period
14.112 r Y 0.150 r 2458256.91970 0.247410300000
ATTENTION: measured mag 10.00 is 4.0 mag brighter than the VSX record maximum brightness 13.96 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:11.46 -13:15:48.6: 10.99 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:11.46 -13:15:48.6: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191112.08-131555.9,2461259.6224,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191112.08-131555.9 20260807.1224 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 10.04 19:11:13.22 -13:23:11.4
23.10923 -10.38199 galactic Sgr Second-epoch detections are separated by 0.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197536723126005504 | 19:11:13.24 -13:23:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.750+/-0.037 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:13.22 -13:23:11.4: 10.97 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:13.22 -13:23:11.4: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197536723126005504,2461259.6224,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197536723126005504 20260807.1224 10.04CV 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 08 07.1224 2461259.6224 9.97 19:11:03.28 -13:20:35.6
23.13115 -10.32693 galactic Sgr Second-epoch detections are separated by 0.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197548817751400192 | 19:11:03.26 -13:20:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.833+/-0.032 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:03.28 -13:20:35.6: 10.90 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:03.28 -13:20:35.6: 11.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.96 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197548817751400192,2461259.6224,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197548817751400192 20260807.1224 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 9.97 19:11:14.96 -13:24:27.2
23.09304 -10.39746 galactic Sgr Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4197536482604852096 | 19:11:14.98 -13:24:27.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.009+/-0.036 (M)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:14.96 -13:24:27.2: 10.89 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:14.96 -13:24:27.2: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4197536482604852096,2461259.6224,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4197536482604852096 20260807.1224 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1224 2461259.6224 9.77 19:10:13.69 -13:13:01.3
23.15811 -10.09100 galactic Sgr Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.5662-13.2177 | 19:10:13.69 -13:13:01.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.803+/-0.043 (K)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:13.69 -13:13:01.3: 10.68 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:13.69 -13:13:01.3: 10.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.5662-13.2177,2461259.6224,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.5662-13.2177 20260807.1224 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461199.80158546 08.06.2026 07:14:06.984 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
First image: 2461199.80158546 08.06.2026 07:14:06.984 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Last image: 2461259.62282243 07.08.2026 02:56:41.858 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.27
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: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17964
Objects passed selection criteria: 17887
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 11350.5
Average stars matched: 10268.2 (90.4652 %)
Memory usage VmPeak: 243852 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 21:59:11 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: 2461199.80158546 08.06.2026 07:14:06.984 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
First image: 2461199.80158546 08.06.2026 07:14:06.984 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Last image: 2461259.62282243 07.08.2026 02:56:41.858 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 121
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.90
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: 35 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 197089
Objects passed selection criteria: 196508
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 127272
Average stars matched: 117639 (92.4308 %)
Memory usage VmPeak: 663916 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 22:00:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
SExtractor catalog cache: saved Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.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/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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: 2461259.62200956
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits exists and is non-empty
Saving wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits to local_wcs_cache/
'wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits'
wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits'
wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits'
wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits (1st reference image)
verification OK: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:40:00.839 -17:58:48.39 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:52.457 -17:59:34.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:00.839 -17:58:48.39
Second-epoch image center 18:39:52.457 -17:59:34.72
Angular distance between the image centers 0.0356 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:51.831 -17:59:01.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:00.839 -17:58:48.39
Second-epoch image center 18:39:51.831 -17:59:01.65
Angular distance between the image centers 0.0359 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:39:52.457 -17:59:34.72
Second-epoch second image center 18:39:51.831 -17:59:01.65
Angular distance between the image centers 0.00951 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/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits &> /tmp/tmp.AG1Dbi7sUL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits &> /tmp/tmp.GBbXcd8WGU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits &> /tmp/tmp.mop3utC1br
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits &> /tmp/tmp.01DcgLfISX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
Found non-empty wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
The reference image (wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits) and catalog (wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat) found
'wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat' -> 'wcsmag.cat'
Read 18477 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5384 to 288.4933 deg, Dec -23.2403 to -12.6035 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 271.5384 to 288.4933 deg, Dec -23.2403 to -12.6035 deg
Loaded 18368 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): 11517 out of 12246 total matches.
Matched with Tycho-2 12246 out of 18477 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.632600
a=0.000000 b=1.000000 c=22.632600
From vast_summary.log: estimated ref. image limiting mag.: -8.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18477 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5384 to 288.4933 deg, Dec -23.2403 to -12.6035 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 271.5384 to 288.4933 deg, Dec -23.2403 to -12.6035 deg
Loaded 18368 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): 11517 out of 12246 total matches.
Matched with Tycho-2 12246 out of 18477 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Forced-photometry filter: calibrated wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits -> calib.txt_param_ref_wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits (aperture=6.3)
Read 22265 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5200 to 288.4473 deg, Dec -23.2260 to -12.5915 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 271.5200 to 288.4473 deg, Dec -23.2260 to -12.5915 deg
Loaded 18299 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): 12510 out of 13428 total matches.
Matched with Tycho-2 13428 out of 22265 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Forced-photometry filter: calibrated wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
2.3 pix Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
2.9 pix fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
3.0 pix fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Limiting magnitude estimates:
14.4 mag. Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
14.5 mag. Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
12.6 mag. fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
12.7 mag. fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.1 (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.AG1Dbi7sUL (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/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits' -> 'wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Checking if the catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS catalog name: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1681, bad_region=0, passed=18477
Got 18477 stars (including 16785 good ones) from the SExtractor catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 18477 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 4810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 18477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 18477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 18477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 4810 stars left (next iteration limit 5289)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits N_match=4810 sigma_overall_arcsec=0.682 sigma_q1_arcsec=0.581 sigma_q2_arcsec=0.723 sigma_q3_arcsec=0.747 sigma_q4_arcsec=0.701 n_q1=1427 n_q2=1157 n_q3=1247 n_q4=979 worst_quadrant_to_overall_ratio=1.096
The image catalog is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits -region wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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.GBbXcd8WGU (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/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits' -> 'wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Checking if the catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS catalog name: wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2015, bad_region=1, passed=22265
Got 22265 stars (including 20226 good ones) from the SExtractor catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 22265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 4809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 22265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 22265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 22265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 4809 stars left (next iteration limit 5289)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits N_match=4809 sigma_overall_arcsec=0.731 sigma_q1_arcsec=0.661 sigma_q2_arcsec=0.902 sigma_q3_arcsec=0.659 sigma_q4_arcsec=0.850 n_q1=1501 n_q2=1080 n_q3=1317 n_q4=911 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits -region wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.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.mop3utC1br (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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=129, bad_region=0, passed=2460
Got 2460 stars (including 2330 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
util/solve_plate_with_UCAC5 got 2460 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (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 0.010453 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 389 (Dec -23.5 to -12.5)
Done reading UCAC5 zone files...
Matched 2278 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2218 matched stars entering correct_measured_positions(), 2209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2218 matched stars entering correct_measured_positions(), 2450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 389 (Dec -23.5 to -12.5)
Done reading UCAC5 zone files...
Matched 2278 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2215 matched stars entering correct_measured_positions(), 2450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 2215 matched stars entering correct_measured_positions(), 2450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 2215 stars left (next iteration limit 2439)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2215 robust_rms=7.211 arcsec worst_quadrant_rms=79.486 arcsec
SIP_REFIT: SIP order 3 trial: matched=2215 robust_rms=0.499 arcsec worst_quadrant_rms=0.577 arcsec
SIP_REFIT: SIP order 5 trial: matched=2215 robust_rms=0.384 arcsec worst_quadrant_rms=0.488 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2215 robust_rms_before=0.737 arcsec robust_rms_before_corrected=0.542 arcsec robust_rms_after=0.384 arcsec worst_quadrant_rms_before=0.777 worst_quadrant_rms_after=0.488
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:52.461 -17:59:35.35 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2460 stars ###
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/correct_sextractor_wcs_catalog_usingxy2sky543292.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.737 -> 0.384 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits N_match=2215 sigma_overall_arcsec=0.412 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.352 n_q1=1140 n_q2=237 n_q3=560 n_q4=278 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits -region wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.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.01DcgLfISX (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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=138, bad_region=0, passed=2505
Got 2505 stars (including 2362 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 2505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (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 0.010453 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.4 to -12.5)
Done reading UCAC5 zone files...
Matched 2304 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2241 matched stars entering correct_measured_positions(), 2230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2241 matched stars entering correct_measured_positions(), 2490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.4 to -12.5)
Done reading UCAC5 zone files...
Matched 2305 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2239 matched stars entering correct_measured_positions(), 2487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 2239 matched stars entering correct_measured_positions(), 2487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 2239 stars left (next iteration limit 2465)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2239 robust_rms=7.767 arcsec worst_quadrant_rms=60.648 arcsec
SIP_REFIT: SIP order 3 trial: matched=2239 robust_rms=0.515 arcsec worst_quadrant_rms=0.590 arcsec
SIP_REFIT: SIP order 5 trial: matched=2239 robust_rms=0.384 arcsec worst_quadrant_rms=0.506 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2239 robust_rms_before=0.748 arcsec robust_rms_before_corrected=0.593 arcsec robust_rms_after=0.384 arcsec worst_quadrant_rms_before=0.925 worst_quadrant_rms_after=0.506
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:51.835 -17:59:02.25 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2505 stars ###
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/correct_sextractor_wcs_catalog_usingxy2sky543196.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.748 -> 0.384 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits N_match=2239 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.397 n_q1=1170 n_q2=220 n_q3=548 n_q4=301 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits -region wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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=Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits sigma_overall=0.682 worst_q_ratio=1.096
ref2=Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits sigma_overall=0.731 worst_q_ratio=1.233
new1=fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits sigma_overall=0.412 worst_q_ratio=1.208
new2=fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits sigma_overall=0.417 worst_q_ratio=1.216
reference average sigma_overall=0.7065 worst_q_ratio=1.1645
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250_astrometric_residuals.png (4810 matched stars from wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.64 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019_astrometric_residuals.png (4809 matched stars from wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.68 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022_astrometric_residuals.png (2215 matched stars from wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023_astrometric_residuals.png (2239 matched stars from wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits'
Preparing the HTML report for the field Sgr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:38:27.27 -12:55:37.7: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:20:35.55 -16:10:48.9: 9.87 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:20:27.66 -16:12:01.2: 9.66 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:55.24 -13:16:13.6: 9.96 +/- 0.00 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:20:27.66 -16:12:01.2: 9.51 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:38:27.27 -12:55:37.7: 15.25 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:20:35.55 -16:10:48.9: 9.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 9.57 +/- 0.01
Forced photometry reference-image weighted average: 9.81 +/- 0.01
Forced photometry filter REJECTED candidate at 18:20:27.66 -16:12:01.2: ref_mag=9.57 +/- 0.01 new_mean_mag=9.7326 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:20:35.55 -16:10:48.9: ref_mag=9.81 +/- 0.01 new_mean_mag=9.9187 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:55.24 -13:16:13.6: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Forced photometry filter KEPT candidate at 19:10:55.24 -13:16:13.6: ref_mag=10.02 +/- 0.00 new_mean_mag=8.9980 delta=1.02 (need > 0.90)
Adding exclusion_list_local.txt__out17221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24302.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24296_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 24296_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24302_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 24302_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24307_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 24307_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17221_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 17221_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16394_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 16394_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:09:24.21 -13:27:26.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03545_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 03545_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:09:45.72 -21:01:26.0 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Sgr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:10:55.24 -13:16:13.6
18:38:27.27 -12:55:37.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
SExtractor catalog cache: saved Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Creating symlink local_wcs_cache/wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits exists and is non-empty
wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits exists and is non-empty
wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits (1st reference image)
verification OK: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:40:00.839 -17:58:48.39 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:52.457 -17:59:34.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:00.839 -17:58:48.39
Second-epoch image center 18:39:52.457 -17:59:34.72
Angular distance between the image centers 0.0356 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:51.831 -17:59:01.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:00.839 -17:58:48.39
Second-epoch image center 18:39:51.831 -17:59:01.65
Angular distance between the image centers 0.0359 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:39:52.457 -17:59:34.72
Second-epoch second image center 18:39:51.831 -17:59:01.65
Angular distance between the image centers 0.00951 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/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits &> /tmp/tmp.B83I43eEjM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits &> /tmp/tmp.Mmdbqq1XWG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits &> /tmp/tmp.7cBg7xUly9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits &> /tmp/tmp.YIIZbra6TW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
Found non-empty wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits and wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
The reference image (wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits) and catalog (wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat) found
'wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat' -> 'wcsmag.cat'
Read 217116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5297 to 288.4971 deg, Dec -23.2473 to -12.5929 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 271.5297 to 288.4971 deg, Dec -23.2473 to -12.5929 deg
Loaded 18407 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): 11784 out of 16173 total matches.
Matched with Tycho-2 16173 out of 217116 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.401950
a=0.000000 b=1.000000 c=22.401950
From vast_summary.log: estimated ref. image limiting mag.: -7.90
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 217116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5297 to 288.4971 deg, Dec -23.2473 to -12.5929 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 271.5297 to 288.4971 deg, Dec -23.2473 to -12.5929 deg
Loaded 18407 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): 11784 out of 16173 total matches.
Matched with Tycho-2 16173 out of 217116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Forced-photometry filter: calibrated wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits -> calib.txt_param_ref_wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits (aperture=4.5)
Read 234793 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.5139 to 288.4713 deg, Dec -23.2286 to -12.5798 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 271.5139 to 288.4713 deg, Dec -23.2286 to -12.5798 deg
Loaded 18361 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): 11742 out of 16151 total matches.
Matched with Tycho-2 16151 out of 234793 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Forced-photometry filter: calibrated wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 79 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
2.2 pix Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
2.5 pix fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
2.5 pix fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Limiting magnitude estimates:
14.5 mag. Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
14.6 mag. Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
12.5 mag. fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
12.6 mag. fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.1 (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.B83I43eEjM (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/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits' -> 'wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
Checking if the catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits
WCS catalog name: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=28509, bad_region=2, passed=217071
Got 217071 stars (including 188330 good ones) from the SExtractor catalog wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 217071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 4809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 217071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 217071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 217071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 4813 stars left (next iteration limit 5288)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits N_match=4813 sigma_overall_arcsec=0.680 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.743 sigma_q3_arcsec=0.741 sigma_q4_arcsec=0.747 n_q1=1419 n_q2=1242 n_q3=1105 n_q4=1047 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits -region wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.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.Mmdbqq1XWG (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/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits' -> 'wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
Checking if the catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits
WCS catalog name: wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=32755, bad_region=5, passed=234752
Got 234752 stars (including 201758 good ones) from the SExtractor catalog wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 234752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 4797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 234752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4793 matched stars entering correct_measured_positions(), 234752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 4793 matched stars entering correct_measured_positions(), 234752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4793 stars left (next iteration limit 5274)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits N_match=4793 sigma_overall_arcsec=0.727 sigma_q1_arcsec=0.629 sigma_q2_arcsec=0.922 sigma_q3_arcsec=0.642 sigma_q4_arcsec=0.889 n_q1=1499 n_q2=1086 n_q3=1245 n_q4=963 worst_quadrant_to_overall_ratio=1.267
The image catalog is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits -region wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.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.7cBg7xUly9 (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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=899, bad_region=0, passed=29255
Got 29255 stars (including 28321 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
util/solve_plate_with_UCAC5 got 29255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (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 0.010453 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 4745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 29252 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4747 matched stars entering correct_measured_positions(), 29253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4747 matched stars entering correct_measured_positions(), 29253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4747 stars left (next iteration limit 5219)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits N_match=4747 sigma_overall_arcsec=0.565 sigma_q1_arcsec=0.680 sigma_q2_arcsec=0.559 sigma_q3_arcsec=0.462 sigma_q4_arcsec=0.464 n_q1=2208 n_q2=482 n_q3=1349 n_q4=708 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits -region wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.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.YIIZbra6TW (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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1178, bad_region=0, passed=30283
Got 30283 stars (including 29061 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 30283 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (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 0.010453 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4754 matched stars entering correct_measured_positions(), 4753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 30280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4750 matched stars entering correct_measured_positions(), 30280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 30280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4749 stars left (next iteration limit 5228)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits N_match=4749 sigma_overall_arcsec=0.565 sigma_q1_arcsec=0.697 sigma_q2_arcsec=0.601 sigma_q3_arcsec=0.463 sigma_q4_arcsec=0.461 n_q1=2227 n_q2=468 n_q3=1288 n_q4=766 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits -region wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-55-31_20.00sec_0.00C_LIGHTs_0022.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.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_2026-08-06_CI_Sgr-02-Q1b1x1_215718_TTUQ1b1x1_532930_jW3C9Yx8/wcs_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023.fits
Preparing the HTML report for the field Sgr-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:16:51.24 -15:57:59.4: 11.87 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:45:43.96 -16:09:53.5: 11.21 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:29:44.29 -16:14:33.2: 11.66 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:40:21.33 -16:26:36.0: 10.57 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:10:50.09 -16:55:03.6: 12.48 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:14:44.12 -18:48:10.0: 11.34 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:15:22.85 -18:42:21.3: 11.19 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:12:47.02 -16:25:52.8: 11.25 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:29:44.29 -16:14:33.2: 11.62 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:16:51.24 -15:57:59.4: 11.73 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:45:43.96 -16:09:53.5: 11.25 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:40:21.33 -16:26:36.0: 10.59 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:10:50.09 -16:55:03.6: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Forced photometry reference-image weighted average: 11.79 +/- 0.02
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Forced photometry reference-image weighted average: 10.58 +/- 0.00
Forced photometry filter REJECTED candidate at 18:29:44.29 -16:14:33.2: ref_mag=11.64 +/- 0.01 new_mean_mag=12.2082 delta=-0.57 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:16:51.24 -15:57:59.4: ref_mag=11.79 +/- 0.02 new_mean_mag=12.0333 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:45:43.96 -16:09:53.5: ref_mag=11.23 +/- 0.01 new_mean_mag=11.7731 delta=-0.54 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:10:50.09 -16:55:03.6: ref_mag=12.39 +/- 0.02 new_mean_mag=12.3542 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:40:21.33 -16:26:36.0: ref_mag=10.58 +/- 0.00 new_mean_mag=11.2922 delta=-0.71 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:14:44.12 -18:48:10.0: 11.31 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:12:47.02 -16:25:52.8: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry filter REJECTED candidate at 18:14:44.12 -18:48:10.0: ref_mag=11.33 +/- 0.01 new_mean_mag=11.2511 delta=0.08 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:15:22.85 -18:42:21.3: 11.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Forced photometry filter REJECTED candidate at 18:12:47.02 -16:25:52.8: ref_mag=11.21 +/- 0.01 new_mean_mag=11.3001 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 11.10 +/- 0.01
Forced photometry filter REJECTED candidate at 18:15:22.85 -18:42:21.3: ref_mag=11.10 +/- 0.01 new_mean_mag=11.1780 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:21:20.77 -16:21:26.1: 11.75 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 18:20:32.77 -16:12:35.2: 12.08 +/- 0.08 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:21:20.77 -16:21:26.1: 11.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.02
Forced photometry filter REJECTED candidate at 18:21:20.77 -16:21:26.1: ref_mag=11.72 +/- 0.02 new_mean_mag=11.8516 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 18:20:32.77 -16:12:35.2: 12.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.06
Forced photometry filter REJECTED candidate at 18:20:32.77 -16:12:35.2: ref_mag=12.05 +/- 0.06 new_mean_mag=12.0177 delta=0.03 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:07:40.65 -13:30:22.0: 12.42 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:06.87 -13:20:30.1: 12.17 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:04.10 -13:31:59.8: 12.47 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:01.82 -13:27:52.0: 12.78 +/- 0.05 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:22.31 -13:22:23.1: 12.47 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:06.87 -13:20:30.1: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:07:40.65 -13:30:22.0: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Forced photometry filter KEPT candidate at 19:10:06.87 -13:20:30.1: ref_mag=12.22 +/- 0.02 new_mean_mag=11.0105 delta=1.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter KEPT candidate at 19:07:40.65 -13:30:22.0: ref_mag=12.45 +/- 0.02 new_mean_mag=11.3463 delta=1.11 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:04.10 -13:31:59.8: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter KEPT candidate at 19:11:04.10 -13:31:59.8: ref_mag=12.53 +/- 0.02 new_mean_mag=11.4028 delta=1.13 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:01.82 -13:27:52.0: 13.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.04
Forced photometry filter KEPT candidate at 19:11:01.82 -13:27:52.0: ref_mag=12.90 +/- 0.04 new_mean_mag=11.5120 delta=1.38 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:46.50 -13:16:03.6: 12.44 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:18.16 -13:35:09.7: 12.43 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:22.31 -13:22:23.1: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:22.31 -13:22:23.1: ref_mag=12.56 +/- 0.02 new_mean_mag=11.4463 delta=1.11 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:37.66 -13:15:13.4: 12.42 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:22.95 -13:12:30.4: 12.39 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:46.50 -13:16:03.6: 12.63 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:18.16 -13:35:09.7: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.03
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter KEPT candidate at 19:10:46.50 -13:16:03.6: ref_mag=12.54 +/- 0.03 new_mean_mag=11.3149 delta=1.23 (need > 0.90)
Forced photometry filter KEPT candidate at 19:11:18.16 -13:35:09.7: ref_mag=12.51 +/- 0.02 new_mean_mag=11.3880 delta=1.12 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:37.66 -13:15:13.4: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:37.66 -13:15:13.4: ref_mag=12.52 +/- 0.02 new_mean_mag=11.4187 delta=1.11 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:57.74 -13:14:24.9: 12.34 +/- 0.04 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:22.95 -13:12:30.4: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:22.95 -13:12:30.4: ref_mag=12.48 +/- 0.02 new_mean_mag=11.3218 delta=1.16 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:57.74 -13:14:24.9: 12.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.03
Forced photometry filter KEPT candidate at 19:10:57.74 -13:14:24.9: ref_mag=12.44 +/- 0.03 new_mean_mag=11.1292 delta=1.31 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:55.89 -13:42:34.7: 12.32 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:55.89 -13:42:34.7: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Forced photometry filter KEPT candidate at 19:08:55.89 -13:42:34.7: ref_mag=12.40 +/- 0.02 new_mean_mag=11.2786 delta=1.12 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:13.22 -13:14:51.2: 12.27 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:13.22 -13:14:51.2: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter KEPT candidate at 19:08:13.22 -13:14:51.2: ref_mag=12.33 +/- 0.02 new_mean_mag=11.2716 delta=1.05 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:06.44 -13:21:22.7: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:06.44 -13:21:22.7: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:06.44 -13:21:22.7: ref_mag=12.36 +/- 0.02 new_mean_mag=11.2821 delta=1.08 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:42.89 -13:47:11.3: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:11.85 -13:40:26.6: 12.20 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:42.89 -13:47:11.3: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:42.89 -13:47:11.3: ref_mag=12.34 +/- 0.02 new_mean_mag=11.2642 delta=1.07 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:08.40 -13:27:27.4: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:39.31 -13:13:01.3: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:11.85 -13:40:26.6: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:11.85 -13:40:26.6: ref_mag=12.28 +/- 0.02 new_mean_mag=11.1783 delta=1.10 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:08.40 -13:27:27.4: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Forced photometry filter KEPT candidate at 19:11:08.40 -13:27:27.4: ref_mag=12.29 +/- 0.02 new_mean_mag=11.2399 delta=1.05 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:39.31 -13:13:01.3: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Forced photometry filter KEPT candidate at 19:08:39.31 -13:13:01.3: ref_mag=12.26 +/- 0.02 new_mean_mag=11.2018 delta=1.06 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:21.18 -13:57:12.8: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:21.18 -13:57:12.8: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter KEPT candidate at 19:11:21.18 -13:57:12.8: ref_mag=12.35 +/- 0.02 new_mean_mag=11.3171 delta=1.04 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:26.78 -13:27:24.7: 12.19 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:26.78 -13:27:24.7: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter KEPT candidate at 19:10:26.78 -13:27:24.7: ref_mag=12.25 +/- 0.02 new_mean_mag=11.0880 delta=1.16 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:33.16 -13:17:20.5: 12.13 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:33.16 -13:17:20.5: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry filter KEPT candidate at 19:08:33.16 -13:17:20.5: ref_mag=12.18 +/- 0.02 new_mean_mag=11.0253 delta=1.15 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:28.49 -13:16:08.4: 12.09 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:28.49 -13:16:08.4: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:28.49 -13:16:08.4: ref_mag=12.18 +/- 0.02 new_mean_mag=11.0880 delta=1.09 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:05.88 -14:31:54.2: 12.10 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:35.28 -13:30:58.1: 12.09 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:05.88 -14:31:54.2: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Forced photometry filter KEPT candidate at 19:11:05.88 -14:31:54.2: ref_mag=12.21 +/- 0.02 new_mean_mag=11.1984 delta=1.01 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:35.28 -13:30:58.1: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:35.28 -13:30:58.1: ref_mag=12.15 +/- 0.02 new_mean_mag=11.1005 delta=1.05 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:07:46.12 -13:56:48.1: 12.03 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:30.55 -13:16:09.0: 12.03 +/- 0.03 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:07:46.12 -13:56:48.1: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.02
Forced photometry filter REJECTED candidate at 19:07:46.12 -13:56:48.1: ref_mag=12.10 +/- 0.02 new_mean_mag=11.2896 delta=0.81 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:30.55 -13:16:09.0: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Forced photometry filter KEPT candidate at 19:10:30.55 -13:16:09.0: ref_mag=12.13 +/- 0.02 new_mean_mag=11.0387 delta=1.10 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:06.81 -13:29:34.4: 11.93 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:40.09 -13:52:20.0: 11.90 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:06.81 -13:29:34.4: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Forced photometry filter KEPT candidate at 19:10:06.81 -13:29:34.4: ref_mag=12.03 +/- 0.02 new_mean_mag=11.0176 delta=1.01 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:40.09 -13:52:20.0: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 19:08:40.09 -13:52:20.0: ref_mag=11.99 +/- 0.01 new_mean_mag=11.0507 delta=0.94 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:08.91 -13:21:07.0: 11.89 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:08.91 -13:21:07.0: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter KEPT candidate at 19:08:08.91 -13:21:07.0: ref_mag=11.95 +/- 0.01 new_mean_mag=10.9686 delta=0.98 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:44.36 -13:20:30.4: 11.85 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:08:58.41 -13:18:06.1: 11.82 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:44.36 -13:20:30.4: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter KEPT candidate at 19:08:44.36 -13:20:30.4: ref_mag=11.94 +/- 0.01 new_mean_mag=10.9476 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:08:58.41 -13:18:06.1: 11.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Forced photometry filter KEPT candidate at 19:08:58.41 -13:18:06.1: ref_mag=11.85 +/- 0.01 new_mean_mag=10.7217 delta=1.13 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:59.67 -13:14:39.9: 11.81 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:59.67 -13:14:39.9: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.02
Forced photometry filter KEPT candidate at 19:09:59.67 -13:14:39.9: ref_mag=11.95 +/- 0.02 new_mean_mag=10.9237 delta=1.03 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:20.17 -13:15:42.9: 11.75 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:20.17 -13:15:42.9: 11.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry filter KEPT candidate at 19:09:20.17 -13:15:42.9: ref_mag=11.82 +/- 0.01 new_mean_mag=10.7332 delta=1.09 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:08.60 -13:25:53.9: 11.64 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:08.60 -13:25:53.9: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:08.60 -13:25:53.9: ref_mag=11.69 +/- 0.01 new_mean_mag=10.7063 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:55.31 -13:14:41.0: 11.65 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:55.31 -13:14:41.0: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:55.31 -13:14:41.0: ref_mag=11.72 +/- 0.01 new_mean_mag=10.6379 delta=1.08 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:49.28 -13:21:25.2: 11.60 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:49.28 -13:21:25.2: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:49.28 -13:21:25.2: ref_mag=11.67 +/- 0.01 new_mean_mag=10.6286 delta=1.04 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:35.49 -13:30:22.3: 11.50 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:09:21.36 -13:19:46.7: 11.50 +/- 0.02 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:35.49 -13:30:22.3: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:35.49 -13:30:22.3: ref_mag=11.55 +/- 0.01 new_mean_mag=10.5614 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:09:21.36 -13:19:46.7: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter KEPT candidate at 19:09:21.36 -13:19:46.7: ref_mag=11.56 +/- 0.01 new_mean_mag=10.5294 delta=1.03 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:04.99 -13:22:06.4: 11.26 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:04.99 -13:22:06.4: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry filter KEPT candidate at 19:11:04.99 -13:22:06.4: ref_mag=11.34 +/- 0.01 new_mean_mag=10.3476 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:11.46 -13:15:48.6: 10.99 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:13.22 -13:23:11.4: 10.97 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:11.46 -13:15:48.6: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.01
Forced photometry filter KEPT candidate at 19:11:11.46 -13:15:48.6: ref_mag=11.08 +/- 0.01 new_mean_mag=9.9991 delta=1.08 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:13.22 -13:23:11.4: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Forced photometry filter KEPT candidate at 19:11:13.22 -13:23:11.4: ref_mag=11.05 +/- 0.01 new_mean_mag=10.0363 delta=1.01 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:03.28 -13:20:35.6: 10.90 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:03.28 -13:20:35.6: 11.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.01
Forced photometry filter KEPT candidate at 19:11:03.28 -13:20:35.6: ref_mag=10.96 +/- 0.01 new_mean_mag=9.9732 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:11:14.96 -13:24:27.2: 10.89 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:11:14.96 -13:24:27.2: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.01
Forced photometry filter KEPT candidate at 19:11:14.96 -13:24:27.2: ref_mag=11.00 +/- 0.01 new_mean_mag=9.9745 delta=1.03 (need > 0.90)
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-06-08_02-14-06_20.00sec_5.00C_LIGHT_0250.fits at 19:10:13.69 -13:13:01.3: 10.68 +/- 0.01 detection
Forced photometry on wcs_Sgr-02-Q1b1x1_2026-07-13_00-53-45_20.00sec_5.00C_LIGHT_0019.fits at 19:10:13.69 -13:13:01.3: 10.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:13.69 -13:13:01.3: ref_mag=10.77 +/- 0.01 new_mean_mag=9.7615 delta=1.01 (need > 0.90)
Adding exclusion_list_local.txt__out167282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out210973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out214001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out214883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out215410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out215658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216594.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 58s
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: 19s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264704_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264704_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264707_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264707_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264711_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264711_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264712_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264712_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264721_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264721_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:37:47.68 -17:15:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264723_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264723_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:14:01.71 -19:10:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264724_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264724_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:11:43.96 -13:32:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264725_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264725_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:20:03.44 -17:05:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264726_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264726_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:19:11.60 -18:03:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264728_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264728_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264731_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264731_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264732_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264732_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264733_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264733_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:18:40.72 -13:46:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264941_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 264941_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265012_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265012_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:17:39.55 -18:01:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265052_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265052_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:17:16.61 -17:21:39.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265053_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265053_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:16:52.71 -16:40:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265098_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265098_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:08:44.97 -21:27:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265108_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265108_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:17:38.73 -19:39:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265111_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265111_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:19:40.40 -18:11:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265112_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265112_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:15:35.53 -18:39:11.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265137_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265137_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:25:26.31 -20:31:24.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265193_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265193_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:14:49.81 -18:48:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265210_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265210_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265235_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265235_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265247_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265247_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:17:16.88 -17:20:46.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265250_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265250_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265334_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 265334_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211503_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 211503_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214883_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 214883_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260729_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 260729_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:38:27.25 -12:55:37.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120549_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 120549_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:21:12.94 -17:32:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234475_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 234475_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:14:57.21 -19:32:14.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213499_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 213499_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215410_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 215410_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211535_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 211535_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210797_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210797_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215658_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 215658_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210612_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210612_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208931_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 208931_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209208_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209208_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167282_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 167282_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209816_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209816_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211380_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 211380_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169270_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 169270_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216594_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 216594_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213295_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 213295_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209190_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209190_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171850_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 171850_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213126_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 213126_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210542_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210542_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210617_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210617_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182932_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 182932_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213937_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 213937_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171549_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 171549_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210380_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210380_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213838_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 213838_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170031_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 170031_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211201_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 211201_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209038_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 209038_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:07:51.81 -13:14:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212333_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212333_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210973_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210973_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209758_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209758_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211088_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 211088_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212506_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212506_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209809_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209809_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212189_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212189_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214001_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 214001_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210730_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210730_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209836_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 209836_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:59:13.16 -13:18:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212093_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212093_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210322_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 210322_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212548_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212548_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212188_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212188_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212618_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 212618_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209225_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 209225_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43102_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 43102_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 18:57:43.69 -21:06:25.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40286_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 40286_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:09:45.75 -21:01:26.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27394_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023
The candidate 27394_fd_Sgr-02-Q1b1x1_2026-08-06_21-56-41_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 19:04:41.01 -21:44:30.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 80s
Prepared the HTML report for the field Sgr-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:10:55.24 -13:16:13.6
18:38:27.27 -12:55:37.7
19:08:55.89 -13:42:34.7
19:09:42.89 -13:47:11.3
19:08:40.09 -13:52:20.0
19:11:21.18 -13:57:12.8
19:11:05.88 -14:31:54.2
19:09:22.95 -13:12:30.4
19:08:39.31 -13:13:01.3
19:10:57.74 -13:14:24.9
19:10:13.69 -13:13:01.3
19:09:59.67 -13:14:39.9
19:10:55.31 -13:14:41.0
19:08:13.22 -13:14:51.2
19:11:11.46 -13:15:48.6
19:10:30.55 -13:16:09.0
19:08:33.16 -13:17:20.5
19:09:37.66 -13:15:13.4
19:09:28.49 -13:16:08.4
19:09:21.36 -13:19:46.7
19:10:46.50 -13:16:03.6
19:08:58.41 -13:18:06.1
19:09:20.17 -13:15:42.9
19:08:08.91 -13:21:07.0
19:09:06.44 -13:21:22.7
19:10:06.87 -13:20:30.1
19:09:22.31 -13:22:23.1
19:11:04.99 -13:22:06.4
19:11:03.28 -13:20:35.6
19:10:49.28 -13:21:25.2
19:08:44.36 -13:20:30.4
19:10:08.60 -13:25:53.9
19:11:13.22 -13:23:11.4
19:11:14.96 -13:24:27.2
19:10:26.78 -13:27:24.7
19:11:08.40 -13:27:27.4
19:11:01.82 -13:27:52.0
19:10:06.81 -13:29:34.4
19:09:35.28 -13:30:58.1
19:10:35.49 -13:30:22.3
19:07:40.65 -13:30:22.0
19:11:04.10 -13:31:59.8
19:11:18.16 -13:35:09.7
19:09:11.85 -13:40:26.6
########### Completed Sgr-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:38:27.27 -12:55:37.7
19:10:55.24 -13:16:13.6
19:10:06.87 -13:20:30.1
19:07:40.65 -13:30:22.0
19:11:01.82 -13:27:52.0
19:11:04.10 -13:31:59.8
19:09:22.31 -13:22:23.1
19:10:46.50 -13:16:03.6
19:11:18.16 -13:35:09.7
19:09:37.66 -13:15:13.4
19:09:22.95 -13:12:30.4
19:10:57.74 -13:14:24.9
19:08:55.89 -13:42:34.7
19:08:13.22 -13:14:51.2
19:09:06.44 -13:21:22.7
19:09:42.89 -13:47:11.3
19:09:11.85 -13:40:26.6
19:11:08.40 -13:27:27.4
19:08:39.31 -13:13:01.3
19:11:21.18 -13:57:12.8
19:10:26.78 -13:27:24.7
19:08:33.16 -13:17:20.5
19:09:28.49 -13:16:08.4
19:11:05.88 -14:31:54.2
19:09:35.28 -13:30:58.1
19:10:30.55 -13:16:09.0
19:10:06.81 -13:29:34.4
19:08:40.09 -13:52:20.0
19:08:08.91 -13:21:07.0
19:08:44.36 -13:20:30.4
19:08:58.41 -13:18:06.1
19:09:59.67 -13:14:39.9
19:09:20.17 -13:15:42.9
19:10:08.60 -13:25:53.9
19:10:55.31 -13:14:41.0
19:10:49.28 -13:21:25.2
19:10:35.49 -13:30:22.3
19:09:21.36 -13:19:46.7
19:11:04.99 -13:22:06.4
19:11:11.46 -13:15:48.6
19:11:13.22 -13:23:11.4
19:11:03.28 -13:20:35.6
19:11:14.96 -13:24:27.2
19:10:13.69 -13:13:01.3
###################################################################################
18:38:27.27 -12:55:37.7 -- asteroid (will NOT add it to exclusion list)
19:10:55.24 -13:16:13.6 -- not an asteroid (will add it to exclusion list)
19:10:06.87 -13:20:30.1 -- not an asteroid (will add it to exclusion list)
19:07:40.65 -13:30:22.0 -- not an asteroid (will add it to exclusion list)
19:11:01.82 -13:27:52.0 -- not an asteroid (will add it to exclusion list)
19:11:04.10 -13:31:59.8 -- not an asteroid (will add it to exclusion list)
19:09:22.31 -13:22:23.1 -- not an asteroid (will add it to exclusion list)
19:10:46.50 -13:16:03.6 -- not an asteroid (will add it to exclusion list)
19:11:18.16 -13:35:09.7 -- not an asteroid (will add it to exclusion list)
19:09:37.66 -13:15:13.4 -- not an asteroid (will add it to exclusion list)
19:09:22.95 -13:12:30.4 -- not an asteroid (will add it to exclusion list)
19:10:57.74 -13:14:24.9 -- not an asteroid (will add it to exclusion list)
19:08:55.89 -13:42:34.7 -- not an asteroid (will add it to exclusion list)
19:08:13.22 -13:14:51.2 -- not an asteroid (will add it to exclusion list)
19:09:06.44 -13:21:22.7 -- not an asteroid (will add it to exclusion list)
19:09:42.89 -13:47:11.3 -- not an asteroid (will add it to exclusion list)
19:09:11.85 -13:40:26.6 -- not an asteroid (will add it to exclusion list)
19:11:08.40 -13:27:27.4 -- not an asteroid (will add it to exclusion list)
19:08:39.31 -13:13:01.3 -- not an asteroid (will add it to exclusion list)
19:11:21.18 -13:57:12.8 -- not an asteroid (will add it to exclusion list)
19:10:26.78 -13:27:24.7 -- not an asteroid (will add it to exclusion list)
19:08:33.16 -13:17:20.5 -- not an asteroid (will add it to exclusion list)
19:09:28.49 -13:16:08.4 -- not an asteroid (will add it to exclusion list)
19:11:05.88 -14:31:54.2 -- not an asteroid (will add it to exclusion list)
19:09:35.28 -13:30:58.1 -- not an asteroid (will add it to exclusion list)
19:10:30.55 -13:16:09.0 -- not an asteroid (will add it to exclusion list)
19:10:06.81 -13:29:34.4 -- not an asteroid (will add it to exclusion list)
19:08:40.09 -13:52:20.0 -- not an asteroid (will add it to exclusion list)
19:08:08.91 -13:21:07.0 -- not an asteroid (will add it to exclusion list)
19:08:44.36 -13:20:30.4 -- not an asteroid (will add it to exclusion list)
19:08:58.41 -13:18:06.1 -- not an asteroid (will add it to exclusion list)
19:09:59.67 -13:14:39.9 -- not an asteroid (will add it to exclusion list)
19:09:20.17 -13:15:42.9 -- not an asteroid (will add it to exclusion list)
19:10:08.60 -13:25:53.9 -- not an asteroid (will add it to exclusion list)
19:10:55.31 -13:14:41.0 -- not an asteroid (will add it to exclusion list)
19:10:49.28 -13:21:25.2 -- not an asteroid (will add it to exclusion list)
19:10:35.49 -13:30:22.3 -- not an asteroid (will add it to exclusion list)
19:09:21.36 -13:19:46.7 -- not an asteroid (will add it to exclusion list)
19:11:04.99 -13:22:06.4 -- not an asteroid (will add it to exclusion list)
19:11:11.46 -13:15:48.6 -- not an asteroid (will add it to exclusion list)
19:11:13.22 -13:23:11.4 -- not an asteroid (will add it to exclusion list)
19:11:03.28 -13:20:35.6 -- not an asteroid (will add it to exclusion list)
19:11:14.96 -13:24:27.2 -- not an asteroid (will add it to exclusion list)
19:10:13.69 -13:13:01.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:07:40.65 -13:30:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:08.91 -13:21:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:13.22 -13:14:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:33.16 -13:17:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:39.31 -13:13:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:40.09 -13:52:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:44.36 -13:20:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:55.89 -13:42:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:58.41 -13:18:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:06.44 -13:21:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:11.85 -13:40:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:20.17 -13:15:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:21.36 -13:19:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:22.31 -13:22:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:22.95 -13:12:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:28.49 -13:16:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:35.28 -13:30:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:37.66 -13:15:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:42.89 -13:47:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:59.67 -13:14:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:06.81 -13:29:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:06.87 -13:20:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:08.60 -13:25:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:13.69 -13:13:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:26.78 -13:27:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:30.55 -13:16:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:35.49 -13:30:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:46.50 -13:16:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:49.28 -13:21:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:55.24 -13:16:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:55.31 -13:14:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:57.74 -13:14:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:01.82 -13:27:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:03.28 -13:20:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:04.10 -13:31:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:04.99 -13:22:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:05.88 -14:31:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:08.40 -13:27:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:11.46 -13:15:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:13.22 -13:23:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:14.96 -13:24:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:18.16 -13:35:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:21.18 -13:57:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:07:40.65 -13:30:22.0 -- not a known variable star
19:08:08.91 -13:21:07.0 -- not a known variable star
19:08:13.22 -13:14:51.2 -- not a known variable star
19:08:33.16 -13:17:20.5 -- not a known variable star
19:08:39.31 -13:13:01.3 -- not a known variable star
19:08:40.09 -13:52:20.0 -- not a known variable star
19:08:44.36 -13:20:30.4 -- not a known variable star
19:08:55.89 -13:42:34.7 -- not a known variable star
19:08:58.41 -13:18:06.1 -- not a known variable star
19:09:06.44 -13:21:22.7 -- not a known variable star
19:09:11.85 -13:40:26.6 -- not a known variable star
19:09:20.17 -13:15:42.9 -- not a known variable star
19:09:21.36 -13:19:46.7 -- not a known variable star
19:09:22.31 -13:22:23.1 -- not a known variable star
19:09:22.95 -13:12:30.4 -- not a known variable star
19:09:28.49 -13:16:08.4 -- not a known variable star
19:09:35.28 -13:30:58.1 -- not a known variable star
19:09:37.66 -13:15:13.4 -- not a known variable star
19:09:42.89 -13:47:11.3 -- not a known variable star
19:09:59.67 -13:14:39.9 -- a known variable star
19:10:06.81 -13:29:34.4 -- not a known variable star
19:10:06.87 -13:20:30.1 -- not a known variable star
19:10:08.60 -13:25:53.9 -- not a known variable star
19:10:13.69 -13:13:01.3 -- not a known variable star
19:10:26.78 -13:27:24.7 -- not a known variable star
19:10:30.55 -13:16:09.0 -- not a known variable star
19:10:35.49 -13:30:22.3 -- not a known variable star
19:10:46.50 -13:16:03.6 -- not a known variable star
19:10:49.28 -13:21:25.2 -- not a known variable star
19:10:55.24 -13:16:13.6 -- not a known variable star
19:10:55.31 -13:14:41.0 -- not a known variable star
19:10:57.74 -13:14:24.9 -- not a known variable star
19:11:01.82 -13:27:52.0 -- not a known variable star
19:11:03.28 -13:20:35.6 -- not a known variable star
19:11:04.10 -13:31:59.8 -- not a known variable star
19:11:04.99 -13:22:06.4 -- not a known variable star
19:11:05.88 -14:31:54.2 -- not a known variable star
19:11:08.40 -13:27:27.4 -- not a known variable star
19:11:11.46 -13:15:48.6 -- a known variable star
19:11:13.22 -13:23:11.4 -- not a known variable star
19:11:14.96 -13:24:27.2 -- not a known variable star
19:11:18.16 -13:35:09.7 -- not a known variable star
19:11:21.18 -13:57:12.8 -- not a known variable star
Found 41 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 43 (excluding asteroids and hot pixels, 41 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461259.62200956 -observatory V36
07:50:50.53 +20:23:11.2 Mercury (-0.4mag)
11:58:53.67 -00:30:28.9 Venus (-4.3mag)
05:46:04.12 +23:34:21.6 Mars (1.3mag)
08:41:56.98 +18:44:58.3 Jupiter (-1.8mag)
00:56:29.64 +03:16:10.6 Saturn (0.6mag)
04:11:36.19 +20:56:37.5 Uranus (5.8mag)
00:16:09.80 +00:13:36.8 Neptune (7.7mag)
20:28:14.79 -23:29:45.3 Pluto (14.4mag)
03:37:53.65 +23:58:06.3 Moon (-10.0mag)
-rw-r--r-- 1 apache apache 363 Aug 6 21:59 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461259.62200956:
08:41:53.08 +18:45:16.4 Io (6.0mag)
08:41:49.56 +18:45:31.4 Europa (6.3mag)
08:42:05.57 +18:44:24.6 Ganymede (5.6mag)
08:41:51.73 +18:45:24.6 Callisto (6.8mag)
08:39:31.82 +18:43:40.8 Himalia (15.7mag)
08:41:59.26 +18:44:48.9 Thebe (16.6mag)
08:39:03.07 +18:42:25.4 Elara (17.7mag)
08:46:03.36 +18:24:57.2 Pasiphae (17.9mag)
08:45:12.22 +18:55:00.2 Carme (19.0mag)
00:56:23.23 +03:16:36.8 Titan (8.4mag)
00:56:25.78 +03:15:58.5 Rhea (9.7mag)
00:56:35.89 +03:14:42.5 Iapetus (11.1mag)
00:56:14.95 +03:16:15.9 Hyperion (14.4mag)
00:55:53.52 +03:09:30.1 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 21:59 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461259.62200956:
18:59:33.26 -23:36:30.4 JWST
18:56:29.77 +17:07:58.5 Chandra
19:39:51.20 +11:52:38.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 21:59 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461259.62200956 -observatory V36
03:12:25.75 +17:17:05.9 17.7mag P/1996 R2 (Lagerkvist)
18:02:07.37 -34:38:07.4 14.0mag P/2010 H2 (Vales)
06:52:45.65 -68:51:35.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:31.68 +32:58:12.6 17.7mag C/2017 K2 (PANSTARRS)
03:40:26.95 +37:09:39.3 16.7mag P/2021 N1 (ZTF)
22:39:32.64 +31:30:53.0 17.3mag C/2022 E2 (ATLAS)
06:42:23.26 +26:33:36.8 16.8mag C/2022 N2 (PANSTARRS)
10:20:32.85 +28:31:08.9 17.0mag C/2022 QE78 (ATLAS)
09:28:07.32 +05:17:54.2 17.9mag C/2022 R6 (PANSTARRS)
15:12:17.33 -12:14:32.3 17.9mag P/2023 B1 (PANSTARRS)
21:12:12.59 +66:08:15.5 17.9mag C/2023 H5 (Lemmon)
15:48:57.38 -12:50:01.3 14.3mag C/2023 R1 (PANSTARRS)
08:06:51.47 +31:17:46.8 15.3mag C/2024 E1 (Wierzchos)
15:07:08.12 +15:36:50.1 17.7mag C/2024 G6 (ATLAS)
19:04:31.33 +43:01:12.7 13.7mag C/2024 J3 (ATLAS)
21:12:21.20 +49:08:22.0 17.6mag C/2024 R4 (PANSTARRS)
05:14:15.23 -12:58:54.0 15.5mag C/2024 T5 (ATLAS)
06:55:30.76 +24:21:01.7 17.9mag C/2025 J1 (Borisov)
07:30:20.72 -15:59:18.8 17.7mag C/2025 R3 (PANSTARRS)
10:31:21.83 +20:58:31.9 17.3mag C/2025 V2 (Rankin)
12:57:28.03 +02:25:24.4 17.0mag C/2025 Y1 (ATLAS)
16:03:21.80 +77:56:14.8 16.8mag C/2026 A2 (Bok)
03:07:05.07 +46:09:52.5 17.1mag C/2026 B2 (Sun-Gao)
11:45:52.80 +08:25:51.9 17.3mag A/2026 E1
21:57:08.71 -26:50:21.1 6.9mag 10P/Tempel
11:28:17.92 -03:19:51.1 16.2mag 29P/Schwassmann-Wachmann
04:37:52.91 +32:20:44.2 18.0mag 47P/Ashbrook-Jackson
11:05:26.60 +05:00:08.3 17.2mag 63P/Wild
00:54:16.52 -05:24:32.7 15.4mag 65P/Gunn
05:33:03.16 +20:43:03.8 13.7mag 78P/Gehrels
20:38:58.75 -23:23:50.8 17.8mag 84P/Giclas
02:59:39.01 +13:36:34.6 16.7mag 88P/Howell
07:53:05.06 +27:48:35.9 16.1mag 93P/Lovas
04:03:13.81 +16:26:39.3 17.6mag 112P/Urata-Niijima
05:52:50.66 +30:25:40.8 16.3mag 114P/Wiseman-Skiff
09:15:53.04 +26:50:12.8 15.0mag 123P/West-Hartley
11:41:31.10 -09:50:42.9 17.1mag 124P/Mrkos
05:34:55.97 +21:11:04.5 16.1mag 128P/Shoemaker-Holt
06:26:38.01 +18:57:16.7 17.9mag 131P/Mueller
00:03:34.52 +03:25:01.6 17.6mag 139P/Vaisala-Oterma
03:21:20.05 -19:42:51.6 14.0mag 161P/Hartley-IRAS
07:12:21.80 +37:44:42.1 15.8mag 162P/SidingSpring
15:34:03.80 +40:12:26.8 12.2mag 169P/NEAT
02:40:59.39 +09:29:41.1 17.6mag 220P/McNaught
16:41:01.52 -10:00:32.4 17.7mag 235P/LINEAR
20:23:07.02 -52:50:54.7 17.8mag 259P/Garradd
03:18:54.14 +24:42:13.3 15.4mag 260P/McNaught
07:02:03.37 +37:44:24.7 17.3mag 295P/LINEAR
15:10:07.27 +03:15:38.1 17.7mag 391P/Kowalski
08:59:52.88 +18:25:49.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 21:59 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
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 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 21:59 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
-rw-r--r-- 1 apache apache 189K Aug 6 21:59 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:56:46.917 -03:48:35.10 AT 2026vtx 2026-06-19.29 21.49
17:22:45.609 +22:50:07.57 AT 2026vtw 2026-05-14.43 21.36
12:21:04.077 -04:01:32.77 AT 2026vtv 2026-02-12.60 20.93
08:14:22.938 +42:27:50.51 AT 2026vtu 2026-01-16.42 20.75
13:48:52.546 -14:32:34.25 AT 2026vtt 2026-05-12.35 21.06
12:45:12.544 +30:35:49.54 SN 2026vts 2026-07-23.20 19.5187
15:54:43.153 +77:05:59.01 AT 2026vtr 2026-07-14.23 20.7687
18:39:56.576 +36:55:41.65 AT 2026vtq 2026-07-15.29 21.179
18:20:04.654 +51:48:07.73 AT 2026vtp 2026-07-12.34 20.506
02:21:08.216 +53:58:20.22 AT 2026vto 2026-07-12.58 18.923
19:18:15.750 -28:25:14.27 AT 2026vtn 2026-07-19.42 19.037
06:18:40.102 -63:52:11.78 AT 2026vtm 2026-07-22.15 18.964
01:25:20.341 +54:04:44.58 AT 2026vtl 2026-07-21.55 18.936
00:31:18.789 +26:35:38.20 AT 2026vtk 2026-07-11.13 18.674
19:17:17.916 -52:23:30.97 AT 2026vtj 2026-07-20.03 18.733
21:18:22.563 -55:04:03.54 AT 2026vti 2026-07-07.91 19.06
13:14:42.843 +01:11:46.35 AT 2026vth 2026-07-07.04 19.288
22:44:00.748 -67:12:53.39 AT 2026vtg 2026-07-22.03 19.382
21:14:49.111 -66:16:14.46 AT 2026vtf 2026-07-19.95 19.278
20:46:38.288 -56:59:08.12 AT 2026vte 2026-07-21.94 18.844
-rw-r--r-- 1 apache apache 87K Aug 6 21:59 tns_transients_list.txt
