This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.21 15:32:11.65 +57:46:41.0
91.68912 48.44066 galactic Dra Second-epoch detections are separated by 0.6" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:32:11.65 +57:46:41.0 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:11.65 +57:46:41.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:11.65 +57:46:41.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.47 15:28:42.32 +58:12:50.8
92.61186 48.61498 galactic Dra Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:42.32 +58:12:50.8 (user input) | T | P | (position from user input) J-Ks=0.754+/-0.027 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:42.32 +58:12:50.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:42.32 +58:12:50.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.26 15:28:34.42 +57:47:33.8
92.07958 48.84867 galactic Dra Second-epoch detections are separated by 0.3" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:34.42 +57:47:33.8 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.029 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:34.42 +57:47:33.8: 13.16 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:34.42 +57:47:33.8: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461245.8693,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.79 15:32:29.58 +58:05:50.8
92.07469 48.24596 galactic Dra Second-epoch detections are separated by 0.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:32:29.58 +58:05:50.8 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.029 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:29.58 +58:05:50.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:29.58 +58:05:50.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461245.8693,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.81 15:31:02.00 +57:59:02.8
92.07476 48.46991 galactic Dra Second-epoch detections are separated by 2.2" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:02.00 +57:59:02.8 (user input) | T | P | (position from user input) J-Ks=0.476+/-0.031 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:02.00 +57:59:02.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:02.00 +57:59:02.8: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461245.8693,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.27 15:29:41.12 +58:06:06.4
92.36527 48.56280 galactic Dra Second-epoch detections are separated by 1.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:29:41.12 +58:06:06.4 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.029 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:41.12 +58:06:06.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:41.12 +58:06:06.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.87 15:31:55.42 +57:52:42.5
91.84726 48.42141 galactic Dra Second-epoch detections are separated by 0.6" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:55.42 +57:52:42.5 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.033 (F)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:55.42 +57:52:42.5: 14.18 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:55.42 +57:52:42.5: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461245.8693,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.93 15:31:54.24 +57:50:46.8
91.80738 48.43983 galactic Dra Second-epoch detections are separated by 0.7" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:54.24 +57:50:46.8 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:54.24 +57:50:46.8: 12.99 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:54.24 +57:50:46.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.29 15:29:53.90 +58:06:11.0
92.34500 48.53804 galactic Dra Second-epoch detections are separated by 0.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:29:53.90 +58:06:11.0 (user input) | T | P | (position from user input) J-Ks=0.696+/-0.028 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:53.90 +58:06:11.0: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:53.90 +58:06:11.0: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.30 15:26:33.11 +58:07:54.9
92.73238 48.89967 galactic Dra Second-epoch detections are separated by 0.2" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:26:33.11 +58:07:54.9 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.028 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:33.11 +58:07:54.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:33.11 +58:07:54.9: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.99 15:35:14.67 +57:56:07.5
91.59284 48.01024 galactic Dra Second-epoch detections are separated by 1.0" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:35:14.67 +57:56:07.5 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.028 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:35:14.67 +57:56:07.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:35:14.67 +57:56:07.5: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.03 15:28:25.23 +58:00:55.0
92.38452 48.75070 galactic Dra Second-epoch detections are separated by 0.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:25.23 +58:00:55.0 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.028 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:25.23 +58:00:55.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:25.23 +58:00:55.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.23 15:31:35.17 +57:58:50.0
92.01410 48.40857 galactic Dra Second-epoch detections are separated by 1.2" and 9.8 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 1602792596986409088 | 15:31:31.11 +57:58:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.030 (F)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:35.17 +57:58:50.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:35.17 +57:58:50.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1602792596986409088,2461245.8693,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1602792596986409088 20260724.3693 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.93 15:34:19.30 +57:53:16.0
91.62085 48.14039 galactic Dra Second-epoch detections are separated by 0.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:34:19.30 +57:53:16.0 (user input) | T | P | (position from user input) J-Ks=0.730+/-0.027 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:34:19.30 +57:53:16.0: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:34:19.30 +57:53:16.0: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461245.8693,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.16 15:28:29.83 +58:00:19.9
92.36388 48.74710 galactic Dra Second-epoch detections are separated by 0.4" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:29.83 +58:00:19.9 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:29.83 +58:00:19.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:29.83 +58:00:19.9: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.61 15:16:47.45 +61:09:03.1
97.53867 48.18557 galactic Dra Second-epoch detections are separated by 3.1" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:16:47.45 +61:09:03.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:16:47.45 +61:09:03.1: 13.80 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:16:47.45 +61:09:03.1: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.24 15:30:43.97 +58:01:32.7
92.15940 48.48294 galactic Dra Second-epoch detections are separated by 0.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:30:43.97 +58:01:32.7 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.027 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:30:43.97 +58:01:32.7: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:30:43.97 +58:01:32.7: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.77 15:30:28.33 +58:06:25.7
92.29149 48.47092 galactic Dra Second-epoch detections are separated by 1.6" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:30:28.33 +58:06:25.7 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.030 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:30:28.33 +58:06:25.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:30:28.33 +58:06:25.7: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.82 15:26:10.02 +58:21:45.0
93.07000 48.81971 galactic Dra Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:26:10.02 +58:21:45.0 (user input) | T | P | (position from user input) J-Ks=0.646+/-0.025 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:10.02 +58:21:45.0: 13.99 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:10.02 +58:21:45.0: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461245.8693,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.90 15:29:21.85 +58:02:11.4
92.31389 48.63287 galactic Dra Second-epoch detections are separated by 0.8" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:29:21.85 +58:02:11.4 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.029 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:21.85 +58:02:11.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:21.85 +58:02:11.4: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.67 15:26:54.72 +58:24:50.8
93.05714 48.70961 galactic Dra Second-epoch detections are separated by 1.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:26:54.72 +58:24:50.8 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.031 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:54.72 +58:24:50.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:54.72 +58:24:50.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461245.8693,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.45 15:31:01.01 +57:47:12.1
91.81956 48.57192 galactic Dra Second-epoch detections are separated by 1.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:01.01 +57:47:12.1 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.040 (F)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:01.01 +57:47:12.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:01.01 +57:47:12.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.83 15:34:23.07 +57:51:26.7
91.57508 48.14808 galactic Dra Second-epoch detections are separated by 0.6" and 9.8 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 J233.5962+57.8573 | 15:34:23.07 +57:51:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.493+/-0.028 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:34:23.07 +57:51:26.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:34:23.07 +57:51:26.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J233.5962+57.8573,2461245.8693,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J233.5962+57.8573 20260724.3693 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.46 15:15:02.43 +61:25:20.5
98.05367 48.18345 galactic Dra Second-epoch detections are separated by 2.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:15:02.43 +61:25:20.5 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:15:02.43 +61:25:20.5: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:15:02.43 +61:25:20.5: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.84 15:29:13.65 +58:01:40.7
92.31699 48.65277 galactic Dra Second-epoch detections are separated by 0.5" and 9.6 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 1602435260003356544 | 15:29:13.64 +58:01:40.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.744+/-0.028 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:13.65 +58:01:40.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:13.65 +58:01:40.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1602435260003356544,2461245.8693,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1602435260003356544 20260724.3693 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.79 15:31:19.51 +58:01:04.5
92.08903 48.41943 galactic Dra Second-epoch detections are separated by 1.8" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:19.51 +58:01:04.5 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.030 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:19.51 +58:01:04.5: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:19.51 +58:01:04.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.88 15:33:12.08 +57:44:22.8
91.53824 48.34329 galactic Dra Second-epoch detections are separated by 1.2" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:33:12.08 +57:44:22.8 (user input) | T | P | (position from user input) J-Ks=0.592+/-0.029 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:33:12.08 +57:44:22.8: 14.24 +/- 0.07 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:33:12.08 +57:44:22.8: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461245.8693,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.73 15:29:58.14 +57:55:47.2
92.11304 48.61904 galactic Dra Second-epoch detections are separated by 1.8" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:29:58.14 +57:55:47.2 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:58.14 +57:55:47.2: 14.10 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:58.14 +57:55:47.2: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461245.8693,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.73CV 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 07 24.3693 2461245.8693 12.65 15:29:53.65 +57:49:15.1
91.97911 48.68332 galactic Dra Second-epoch detections are separated by 0.8" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J232.4770+57.8216 | 15:29:53.65 +57:49:15.1 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.492+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:53.65 +57:49:15.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:53.65 +57:49:15.1: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J232.4770+57.8216,2461245.8693,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J232.4770+57.8216 20260724.3693 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.54 15:28:46.22 +58:00:43.4
92.34385 48.71279 galactic Dra Second-epoch detections are separated by 0.6" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:46.22 +58:00:43.4 (user input) | T | P | (position from user input) J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:46.22 +58:00:43.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:46.22 +58:00:43.4: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461245.8693,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 11.85 15:29:44.94 +57:50:06.0
92.01248 48.69269 galactic Dra Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1602416877543361280 | 15:29:44.94 +57:50:06.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.609+/-0.029 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:44.94 +57:50:06.0: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:44.94 +57:50:06.0: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1602416877543361280,2461245.8693,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1602416877543361280 20260724.3693 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.32 15:27:30.97 +58:11:41.7
92.71153 48.75842 galactic Dra Second-epoch detections are separated by 0.7" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:27:30.97 +58:11:41.7 (user input) | T | P | (position from user input) J-Ks=0.551+/-0.025 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:30.97 +58:11:41.7: 13.37 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:30.97 +58:11:41.7: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.28 15:31:18.25 +57:57:46.2
92.01962 48.44978 galactic Dra Second-epoch detections are separated by 1.3" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:18.25 +57:57:46.2 (user input) | T | P | (position from user input) J-Ks=0.476+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:18.25 +57:57:46.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:18.25 +57:57:46.2: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.86 15:31:08.90 +58:07:10.6
92.23882 48.38781 galactic Dra Second-epoch detections are separated by 1.1" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:31:08.90 +58:07:10.6 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.035 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:08.90 +58:07:10.6: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:08.90 +58:07:10.6: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461245.8693,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.43 15:26:20.38 +58:08:45.4
92.77307 48.91596 galactic Dra Second-epoch detections are separated by 0.5" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:26:20.38 +58:08:45.4 (user input) | T | P | (position from user input) J-Ks=0.571+/-0.028 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:20.38 +58:08:45.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:20.38 +58:08:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.22 15:29:55.55 +57:54:09.2
92.08211 48.63791 galactic Dra Second-epoch detections are separated by 1.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:29:55.55 +57:54:09.2 (user input) | T | P | (position from user input) J-Ks=0.571+/-0.029 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:55.55 +57:54:09.2: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:55.55 +57:54:09.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.19 15:27:39.76 +58:06:07.6
92.57633 48.79078 galactic Dra Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:27:39.76 +58:06:07.6 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:39.76 +58:06:07.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:39.76 +58:06:07.6: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.26 15:32:12.47 +57:45:53.4
91.67049 48.44569 galactic Dra Second-epoch detections are separated by 0.8" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:32:12.47 +57:45:53.4 (user input) | T | P | (position from user input) J-Ks=0.630+/-0.030 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:12.47 +57:45:53.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:12.47 +57:45:53.4: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.32 15:32:01.20 +57:47:50.0
91.73166 48.45114 galactic Dra Second-epoch detections are separated by 0.5" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:32:01.20 +57:47:50.0 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.028 (K)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:01.20 +57:47:50.0: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:01.20 +57:47:50.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.52 15:31:07.95 +57:46:01.5
91.78221 48.56853 galactic Dra Second-epoch detections are separated by 1.6" and 9.9 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 J232.7911+57.7657 | 15:31:07.95 +57:46:01.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.396+/-0.030 (G)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:07.95 +57:46:01.5: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:07.95 +57:46:01.5: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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
ATO J232.7911+57.7657,2461245.8693,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J232.7911+57.7657 20260724.3693 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 24.3693 2461245.8693 12.62 15:27:01.09 +58:15:05.3
92.83694 48.78420 galactic Dra Second-epoch detections are separated by 1.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:27:01.09 +58:15:05.3 (user input) | T | P | (position from user input) J-Ks=0.285+/-0.030 (F)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:01.09 +58:15:05.3: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:01.09 +58:15:05.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461245.8693,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260724.3693 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461199.78168939 08.06.2026 06:45:27.963 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
First image: 2461199.78168939 08.06.2026 06:45:27.963 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Last image: 2461245.86963566 24.07.2026 08:52:06.521 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6209
Objects passed selection criteria: 6157
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 3556.5
Average stars matched: 3469.75 (97.5608 %)
Memory usage VmPeak: 116008 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 23 15:05:06 CDT 2026
VaST build number 1.0rc89-167-gea1982e4
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-23)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 24 06:06:14 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: 2461199.78168939 08.06.2026 06:45:27.963 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
First image: 2461199.78168939 08.06.2026 06:45:27.963 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Last image: 2461245.86963566 24.07.2026 08:52:06.521 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 33784
Objects passed selection criteria: 33642
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 20220.8
Average stars matched: 19508.8 (96.4789 %)
Memory usage VmPeak: 142224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 23 15:05:06 CDT 2026
VaST build number 1.0rc89-167-gea1982e4
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-23)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 24 06:08:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
SExtractor catalog cache: saved Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.cat to cache
SExtractor catalog cache: saved Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.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/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.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: 2461245.86892000
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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits exists and is non-empty
Saving wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits to local_wcs_cache/
'wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits' -> 'local_wcs_cache/wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits'
wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits exists and is non-empty
Saving wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits to local_wcs_cache/
'wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits' -> 'local_wcs_cache/wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits'
wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits exists and is non-empty
Saving wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits to local_wcs_cache/
'wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits' -> 'local_wcs_cache/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits'
wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits exists and is non-empty
Saving wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits to local_wcs_cache/
'wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits (1st reference image)
verification OK: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:39.841 +62:00:40.47 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_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits (1st new image)
verification OK: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Image size: 937.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:40.926 +62:00:10.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:39.841 +62:00:40.47
Second-epoch image center 15:25:40.926 +62:00:10.48
Angular distance between the image centers 0.0086 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits (2nd new image)
verification OK: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:35.833 +61:59:28.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:39.841 +62:00:40.47
Second-epoch image center 15:25:35.833 +61:59:28.67
Angular distance between the image centers 0.0214 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 15:25:40.926 +62:00:10.48
Second-epoch second image center 15:25:35.833 +61:59:28.67
Angular distance between the image centers 0.01530 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/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits &> /tmp/tmp.PvK7Ccu1xG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits &> /tmp/tmp.xRJmHXG2co
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits &> /tmp/tmp.KI8sGfP3mB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits &> /tmp/tmp.hocUqxtEfb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
Found non-empty wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
The reference image (wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits) and catalog (wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat) found
'wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat' -> 'wcsmag.cat'
Read 8441 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.2399 to 250.7073 deg, Dec +55.9126 to +67.2630 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 212.2399 to 250.7073 deg, Dec 55.9126 to 67.2630 deg
Loaded 7130 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): 4750 out of 4923 total matches.
Matched with Tycho-2 4923 out of 8441 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.680600
a=0.000000 b=1.000000 c=22.680600
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8441 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.2399 to 250.7073 deg, Dec +55.9126 to +67.2630 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 212.2399 to 250.7073 deg, Dec 55.9126 to 67.2630 deg
Loaded 7130 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): 4750 out of 4923 total matches.
Matched with Tycho-2 4923 out of 8441 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits:
Forced-photometry filter: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits -> calib.txt_param_ref_wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits (aperture=6.3)
Read 8392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.2396 to 250.7351 deg, Dec +55.9126 to +67.2632 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 212.2396 to 250.7351 deg, Dec 55.9126 to 67.2632 deg
Loaded 7138 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): 4750 out of 4914 total matches.
Matched with Tycho-2 4914 out of 8392 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits:
Forced-photometry filter: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits -> calib.txt_param_ref_wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
2.3 pix Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
2.4 pix fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
2.3 pix fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
2.3 pix wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
2.3 pix wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Limiting magnitude estimates:
15.3 mag. Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
15.3 mag. Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
13.1 mag. fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
12.8 mag. fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.3 (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.PvK7Ccu1xG (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits' -> 'wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Checking if the catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS catalog name: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=506, bad_region=1819, passed=8441
Got 8441 stars (including 6205 good ones) from the SExtractor catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
util/solve_plate_with_UCAC5 got 8441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits N_match=971 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.326 n_q1=315 n_q2=198 n_q3=303 n_q4=155 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits -region wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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.xRJmHXG2co (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits' -> 'wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS-calibrated image found: wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Checking if the catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS catalog name: wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=489, bad_region=1827, passed=8392
Got 8392 stars (including 6177 good ones) from the SExtractor catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 8392 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits N_match=969 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.472 sigma_q4_arcsec=0.374 n_q1=319 n_q2=193 n_q3=304 n_q4=153 worst_quadrant_to_overall_ratio=1.255
The image catalog is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits -region wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.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.KI8sGfP3mB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS-calibrated image found: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Checking if the catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS catalog name: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=36, bad_region=168, passed=772
Got 772 stars (including 577 good ones) from the SExtractor catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 787 (Dec 56.1 to 67.2)
Done reading UCAC5 zone files...
Matched 550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 550 matched stars entering correct_measured_positions(), 525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 550 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 787 (Dec 56.1 to 67.2)
Done reading UCAC5 zone files...
Matched 550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 550 matched stars entering correct_measured_positions(), 579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 550 matched stars entering correct_measured_positions(), 579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 550 stars left (next iteration limit 605)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits N_match=550 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.620 sigma_q2_arcsec=1.007 sigma_q3_arcsec=0.613 sigma_q4_arcsec=0.456 n_q1=211 n_q2=46 n_q3=120 n_q4=173 worst_quadrant_to_overall_ratio=1.764
The image catalog is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits -region wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.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.hocUqxtEfb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Checking if the catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS catalog name: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=27, bad_region=218, passed=744
Got 744 stars (including 507 good ones) from the SExtractor catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.2)
Done reading UCAC5 zone files...
Matched 490 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 490 matched stars entering correct_measured_positions(), 457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 490 matched stars entering correct_measured_positions(), 493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.2)
Done reading UCAC5 zone files...
Matched 490 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 490 matched stars entering correct_measured_positions(), 489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 490 matched stars entering correct_measured_positions(), 489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 490 stars left (next iteration limit 539)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits N_match=490 sigma_overall_arcsec=0.508 sigma_q1_arcsec=0.782 sigma_q2_arcsec=0.705 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.438 n_q1=135 n_q2=43 n_q3=176 n_q4=136 worst_quadrant_to_overall_ratio=1.541
The image catalog is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits -region wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.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=Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits sigma_overall=0.353 worst_q_ratio=1.147
ref2=Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits sigma_overall=0.376 worst_q_ratio=1.255
new1=fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits sigma_overall=0.571 worst_q_ratio=1.764
new2=fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits sigma_overall=0.508 worst_q_ratio=1.541
reference average sigma_overall=0.3645 worst_q_ratio=1.201
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215_astrometric_residuals.png (971 matched stars from wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216_astrometric_residuals.png (969 matched stars from wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199_astrometric_residuals.png (550 matched stars from wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200_astrometric_residuals.png (490 matched stars from wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits'
Saving fully-calibrated image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits'
Preparing the HTML report for the field Dra-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
SExtractor catalog cache: saved Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.cat to cache
SExtractor catalog cache: saved Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Creating symlink local_wcs_cache/wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits exists and is non-empty
wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits exists and is non-empty
wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits exists and is non-empty
wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits (1st reference image)
verification OK: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:39.841 +62:00:40.47 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_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits (1st new image)
verification OK: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Image size: 937.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:40.926 +62:00:10.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:39.841 +62:00:40.47
Second-epoch image center 15:25:40.926 +62:00:10.48
Angular distance between the image centers 0.0086 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits (2nd new image)
verification OK: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Image size: 937.7'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:35.833 +61:59:28.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:39.841 +62:00:40.47
Second-epoch image center 15:25:35.833 +61:59:28.67
Angular distance between the image centers 0.0214 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 15:25:40.926 +62:00:10.48
Second-epoch second image center 15:25:35.833 +61:59:28.67
Angular distance between the image centers 0.01530 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/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits &> /tmp/tmp.xWp1zLIAgg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits &> /tmp/tmp.wsuqWwbBxt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits &> /tmp/tmp.eNLa0XUXFr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits &> /tmp/tmp.nhk7LTYIbR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
Found non-empty wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits and wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
The reference image (wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits) and catalog (wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat) found
'wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat' -> 'wcsmag.cat'
Read 43673 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.1532 to 251.0204 deg, Dec +55.8917 to +67.2772 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 212.1532 to 251.0204 deg, Dec 55.8917 to 67.2772 deg
Loaded 7252 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): 4534 out of 4976 total matches.
Matched with Tycho-2 4976 out of 43673 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.562250
a=0.000000 b=1.000000 c=22.562250
From vast_summary.log: estimated ref. image limiting mag.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 43673 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.1532 to 251.0204 deg, Dec +55.8917 to +67.2772 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 212.1532 to 251.0204 deg, Dec 55.8917 to 67.2772 deg
Loaded 7252 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): 4534 out of 4976 total matches.
Matched with Tycho-2 4976 out of 43673 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits:
Forced-photometry filter: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits -> calib.txt_param_ref_wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits (aperture=4.9)
Read 43634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 212.1519 to 250.9030 deg, Dec +55.8920 to +67.2680 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 212.1519 to 250.9030 deg, Dec 55.8920 to 67.2680 deg
Loaded 7219 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): 4534 out of 4975 total matches.
Matched with Tycho-2 4975 out of 43634 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits:
Forced-photometry filter: calibrated wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits -> calib.txt_param_ref_wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
2.2 pix Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
2.3 pix fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
2.2 pix fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
2.2 pix wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
2.2 pix wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Limiting magnitude estimates:
15.5 mag. Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
15.5 mag. Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
13.1 mag. fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
13.0 mag. fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (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.xWp1zLIAgg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits' -> 'wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
Checking if the catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits
WCS catalog name: wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2064, bad_region=6994, passed=43656
Got 43656 stars (including 34917 good ones) from the SExtractor catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat
util/solve_plate_with_UCAC5 got 43656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 37568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 37569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 37569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits N_match=970 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.359 n_q1=328 n_q2=197 n_q3=290 n_q4=155 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits -region wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.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.wsuqWwbBxt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits' -> 'wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS-calibrated image found: wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
Checking if the catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat corresponding to the image wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits
WCS catalog name: wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2012, bad_region=6972, passed=43612
Got 43612 stars (including 34952 good ones) from the SExtractor catalog wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 43612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 37588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 37588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 37588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits N_match=968 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.390 n_q1=326 n_q2=194 n_q3=292 n_q4=156 worst_quadrant_to_overall_ratio=1.131
The image catalog is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits -region wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.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.eNLa0XUXFr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS-calibrated image found: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Checking if the catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
WCS catalog name: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=196, bad_region=659, passed=4925
Got 4925 stars (including 4147 good ones) from the SExtractor catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 4925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits N_match=952 sigma_overall_arcsec=0.581 sigma_q1_arcsec=0.601 sigma_q2_arcsec=0.876 sigma_q3_arcsec=0.576 sigma_q4_arcsec=0.517 n_q1=389 n_q2=79 n_q3=216 n_q4=268 worst_quadrant_to_overall_ratio=1.507
The image catalog is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits -region wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.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.nhk7LTYIbR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Checking if the catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
WCS catalog name: wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=162, bad_region=837, passed=4723
Got 4723 stars (including 3814 good ones) from the SExtractor catalog wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 4723 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.2)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 3820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.2)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 3818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 3818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits N_match=953 sigma_overall_arcsec=0.503 sigma_q1_arcsec=0.821 sigma_q2_arcsec=0.602 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.423 n_q1=291 n_q2=83 n_q3=338 n_q4=241 worst_quadrant_to_overall_ratio=1.633
The image catalog is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits -region wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.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_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-51-04_20.00sec_4.90C_LIGHT_0199.fits
Saving fully-calibrated image wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-24_CI_Dra-06-Q2b1x1_040904_TTUQ2b1x1_1121360_L9DX7Bwd/wcs_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200.fits
Preparing the HTML report for the field Dra-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:54.24 +57:50:46.8: 12.99 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:34.42 +57:47:33.8: 13.16 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:41.12 +58:06:06.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:11.65 +57:46:41.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:29.58 +58:05:50.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:42.32 +58:12:50.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:55.42 +57:52:42.5: 14.18 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:33.11 +58:07:54.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:02.00 +57:59:02.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:53.90 +58:06:11.0: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:54.24 +57:50:46.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 15:31:54.24 +57:50:46.8: ref_mag=12.99 +/- 0.02 new_mean_mag=11.9323 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:41.12 +58:06:06.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:11.65 +57:46:41.0: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:34.42 +57:47:33.8: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:33.11 +58:07:54.9: 13.33 +/- 0.03 detection
Forced photometry filter KEPT candidate at 15:29:41.12 +58:06:06.4: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2395 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:02.00 +57:59:02.8: 14.15 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:29.58 +58:05:50.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 15:28:34.42 +57:47:33.8: ref_mag=13.14 +/- 0.02 new_mean_mag=12.2105 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:42.32 +58:12:50.8: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:55.42 +57:52:42.5: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 15:32:11.65 +57:46:41.0: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2017 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:53.90 +58:06:11.0: 13.28 +/- 0.03 detection
Forced photometry filter KEPT candidate at 15:26:33.11 +58:07:54.9: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2590 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter KEPT candidate at 15:31:02.00 +57:59:02.8: ref_mag=14.08 +/- 0.04 new_mean_mag=12.8132 delta=1.26 (need > 0.90)
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 15:32:29.58 +58:05:50.8: ref_mag=13.82 +/- 0.03 new_mean_mag=12.7629 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 15:31:55.42 +57:52:42.5: ref_mag=14.15 +/- 0.04 new_mean_mag=12.8760 delta=1.27 (need > 0.90)
Forced photometry filter KEPT candidate at 15:28:42.32 +58:12:50.8: ref_mag=13.41 +/- 0.02 new_mean_mag=12.4421 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 15:29:53.90 +58:06:11.0: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2869 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:35:14.67 +57:56:07.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:35:14.67 +57:56:07.5: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 15:35:14.67 +57:56:07.5: ref_mag=12.98 +/- 0.02 new_mean_mag=11.9801 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:25.23 +58:00:55.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:35.17 +57:58:50.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:34:19.30 +57:53:16.0: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:25.23 +58:00:55.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 15:28:25.23 +58:00:55.0: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0377 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:35.17 +57:58:50.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 15:31:35.17 +57:58:50.0: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2467 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:29.83 +58:00:19.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:34:19.30 +57:53:16.0: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:16:47.45 +61:09:03.1: 13.80 +/- 0.04 detection
Forced photometry filter KEPT candidate at 15:34:19.30 +57:53:16.0: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9018 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:29.83 +58:00:19.9: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 15:28:29.83 +58:00:19.9: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1671 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:30:43.97 +58:01:32.7: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:16:47.45 +61:09:03.1: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 15:16:47.45 +61:09:03.1: ref_mag=13.78 +/- 0.03 new_mean_mag=12.5861 delta=1.20 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:30:28.33 +58:06:25.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:10.02 +58:21:45.0: 13.99 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:30:43.97 +58:01:32.7: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 15:30:43.97 +58:01:32.7: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2424 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:21.85 +58:02:11.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:10.02 +58:21:45.0: 13.94 +/- 0.05 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:30:28.33 +58:06:25.7: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 15:26:10.02 +58:21:45.0: ref_mag=13.96 +/- 0.04 new_mean_mag=12.8161 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 15:30:28.33 +58:06:25.7: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7684 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:21.85 +58:02:11.4: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 15:29:21.85 +58:02:11.4: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9122 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:54.72 +58:24:50.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:54.72 +58:24:50.8: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 15:26:54.72 +58:24:50.8: ref_mag=13.73 +/- 0.03 new_mean_mag=12.6728 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:01.01 +57:47:12.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:34:23.07 +57:51:26.7: 12.86 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:15:02.43 +61:25:20.5: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:01.01 +57:47:12.1: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:13.65 +58:01:40.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 15:31:01.01 +57:47:12.1: ref_mag=13.66 +/- 0.03 new_mean_mag=12.4704 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:34:23.07 +57:51:26.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 15:34:23.07 +57:51:26.7: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8244 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:15:02.43 +61:25:20.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:19.51 +58:01:04.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 15:15:02.43 +61:25:20.5: ref_mag=13.47 +/- 0.02 new_mean_mag=12.4477 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:13.65 +58:01:40.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 15:29:13.65 +58:01:40.7: ref_mag=12.84 +/- 0.01 new_mean_mag=11.8375 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:19.51 +58:01:04.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 15:31:19.51 +58:01:04.5: ref_mag=13.85 +/- 0.03 new_mean_mag=12.7395 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:33:12.08 +57:44:22.8: 14.24 +/- 0.07 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:33:12.08 +57:44:22.8: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 15:33:12.08 +57:44:22.8: ref_mag=14.12 +/- 0.04 new_mean_mag=12.8923 delta=1.23 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:58.14 +57:55:47.2: 14.10 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:53.65 +57:49:15.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:28:46.22 +58:00:43.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:58.14 +57:55:47.2: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 15:29:58.14 +57:55:47.2: ref_mag=14.10 +/- 0.04 new_mean_mag=12.7334 delta=1.37 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:53.65 +57:49:15.1: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter KEPT candidate at 15:29:53.65 +57:49:15.1: ref_mag=13.82 +/- 0.03 new_mean_mag=12.6357 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:28:46.22 +58:00:43.4: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 15:28:46.22 +58:00:43.4: ref_mag=13.73 +/- 0.03 new_mean_mag=12.5482 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:44.94 +57:50:06.0: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:30.97 +58:11:41.7: 13.37 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:44.94 +57:50:06.0: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 15:29:44.94 +57:50:06.0: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8462 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:30.97 +58:11:41.7: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 15:27:30.97 +58:11:41.7: ref_mag=13.38 +/- 0.02 new_mean_mag=12.2847 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:18.25 +57:57:46.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:18.25 +57:57:46.2: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 15:31:18.25 +57:57:46.2: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2895 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:08.90 +58:07:10.6: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:26:20.38 +58:08:45.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:29:55.55 +57:54:09.2: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:08.90 +58:07:10.6: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry filter KEPT candidate at 15:31:08.90 +58:07:10.6: ref_mag=14.09 +/- 0.04 new_mean_mag=12.8623 delta=1.23 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:39.76 +58:06:07.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:26:20.38 +58:08:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 15:26:20.38 +58:08:45.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3861 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:12.47 +57:45:53.4: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:29:55.55 +57:54:09.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 15:29:55.55 +57:54:09.2: ref_mag=13.35 +/- 0.02 new_mean_mag=12.2143 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:32:01.20 +57:47:50.0: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:39.76 +58:06:07.6: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 15:27:39.76 +58:06:07.6: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1536 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:12.47 +57:45:53.4: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 15:32:12.47 +57:45:53.4: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2645 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:32:01.20 +57:47:50.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Forced photometry filter KEPT candidate at 15:32:01.20 +57:47:50.0: ref_mag=13.48 +/- 0.02 new_mean_mag=12.3259 delta=1.15 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:31:07.95 +57:46:01.5: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:31:07.95 +57:46:01.5: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 15:31:07.95 +57:46:01.5: ref_mag=13.54 +/- 0.03 new_mean_mag=12.5038 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-45-27_20.00sec_4.90C_LIGHT_0215.fits at 15:27:01.09 +58:15:05.3: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-06-Q2b1x1_2026-06-08_01-46-13_20.00sec_4.90C_LIGHT_0216.fits at 15:27:01.09 +58:15:05.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 15:27:01.09 +58:15:05.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.6258 delta=1.06 (need > 0.90)
Adding exclusion_list_local.txt__out25054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34893.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 74s
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: 21s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32252_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32252_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34110_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 34110_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32198_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32198_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33669_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33669_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33163_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33163_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33496_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33496_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32682_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32682_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32586_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32586_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33542_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33542_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33711_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33711_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32984_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32984_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33265_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33265_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33154_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33154_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32702_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32702_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33179_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33179_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26262_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 26262_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33269_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33269_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33670_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33670_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34705_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 34705_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32948_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32948_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34893_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 34893_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32216_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32216_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32637_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32637_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25054_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 25054_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33094_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33094_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33118_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33118_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32172_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32172_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32929_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32929_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32340_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32340_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33172_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33172_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32379_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32379_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33949_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33949_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32859_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32859_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33738_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33738_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33749_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33749_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32743_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32743_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33443_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 33443_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31803_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 31803_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32360_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32360_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32175_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 32175_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34234_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
Preparing report for the candidate 34234_fd_Dra-06-Q2b1x1_2026-07-24_03-52-06_20.00sec_4.90C_LIGHT_0200
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 98s
Prepared the HTML report for the field Dra-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:15:02.43 +61:25:20.5
15:16:47.45 +61:09:03.1
15:32:12.47 +57:45:53.4
15:33:12.08 +57:44:22.8
15:31:07.95 +57:46:01.5
15:28:34.42 +57:47:33.8
15:31:01.01 +57:47:12.1
15:32:11.65 +57:46:41.0
15:29:53.65 +57:49:15.1
15:32:01.20 +57:47:50.0
15:29:44.94 +57:50:06.0
15:31:54.24 +57:50:46.8
15:34:23.07 +57:51:26.7
15:31:55.42 +57:52:42.5
15:34:19.30 +57:53:16.0
15:29:55.55 +57:54:09.2
15:31:18.25 +57:57:46.2
15:29:58.14 +57:55:47.2
15:29:21.85 +58:02:11.4
15:35:14.67 +57:56:07.5
15:29:13.65 +58:01:40.7
15:31:19.51 +58:01:04.5
15:31:35.17 +57:58:50.0
15:31:02.00 +57:59:02.8
15:28:46.22 +58:00:43.4
15:28:29.83 +58:00:19.9
15:28:25.23 +58:00:55.0
15:30:43.97 +58:01:32.7
15:27:39.76 +58:06:07.6
15:29:41.12 +58:06:06.4
15:29:53.90 +58:06:11.0
15:32:29.58 +58:05:50.8
15:30:28.33 +58:06:25.7
15:26:33.11 +58:07:54.9
15:31:08.90 +58:07:10.6
15:26:20.38 +58:08:45.4
15:27:30.97 +58:11:41.7
15:28:42.32 +58:12:50.8
15:27:01.09 +58:15:05.3
15:26:10.02 +58:21:45.0
15:26:54.72 +58:24:50.8
########### Completed Dra-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
15:32:11.65 +57:46:41.0
15:28:42.32 +58:12:50.8
15:28:34.42 +57:47:33.8
15:32:29.58 +58:05:50.8
15:31:02.00 +57:59:02.8
15:29:41.12 +58:06:06.4
15:31:55.42 +57:52:42.5
15:31:54.24 +57:50:46.8
15:29:53.90 +58:06:11.0
15:26:33.11 +58:07:54.9
15:35:14.67 +57:56:07.5
15:28:25.23 +58:00:55.0
15:31:35.17 +57:58:50.0
15:34:19.30 +57:53:16.0
15:28:29.83 +58:00:19.9
15:16:47.45 +61:09:03.1
15:30:43.97 +58:01:32.7
15:30:28.33 +58:06:25.7
15:26:10.02 +58:21:45.0
15:29:21.85 +58:02:11.4
15:26:54.72 +58:24:50.8
15:31:01.01 +57:47:12.1
15:34:23.07 +57:51:26.7
15:15:02.43 +61:25:20.5
15:29:13.65 +58:01:40.7
15:31:19.51 +58:01:04.5
15:33:12.08 +57:44:22.8
15:29:58.14 +57:55:47.2
15:29:53.65 +57:49:15.1
15:28:46.22 +58:00:43.4
15:29:44.94 +57:50:06.0
15:27:30.97 +58:11:41.7
15:31:18.25 +57:57:46.2
15:31:08.90 +58:07:10.6
15:26:20.38 +58:08:45.4
15:29:55.55 +57:54:09.2
15:27:39.76 +58:06:07.6
15:32:12.47 +57:45:53.4
15:32:01.20 +57:47:50.0
15:31:07.95 +57:46:01.5
15:27:01.09 +58:15:05.3
###################################################################################
15:32:11.65 +57:46:41.0 -- not an asteroid (will add it to exclusion list)
15:28:42.32 +58:12:50.8 -- not an asteroid (will add it to exclusion list)
15:28:34.42 +57:47:33.8 -- not an asteroid (will add it to exclusion list)
15:32:29.58 +58:05:50.8 -- not an asteroid (will add it to exclusion list)
15:31:02.00 +57:59:02.8 -- not an asteroid (will add it to exclusion list)
15:29:41.12 +58:06:06.4 -- not an asteroid (will add it to exclusion list)
15:31:55.42 +57:52:42.5 -- not an asteroid (will add it to exclusion list)
15:31:54.24 +57:50:46.8 -- not an asteroid (will add it to exclusion list)
15:29:53.90 +58:06:11.0 -- not an asteroid (will add it to exclusion list)
15:26:33.11 +58:07:54.9 -- not an asteroid (will add it to exclusion list)
15:35:14.67 +57:56:07.5 -- not an asteroid (will add it to exclusion list)
15:28:25.23 +58:00:55.0 -- not an asteroid (will add it to exclusion list)
15:31:35.17 +57:58:50.0 -- not an asteroid (will add it to exclusion list)
15:34:19.30 +57:53:16.0 -- not an asteroid (will add it to exclusion list)
15:28:29.83 +58:00:19.9 -- not an asteroid (will add it to exclusion list)
15:16:47.45 +61:09:03.1 -- not an asteroid (will add it to exclusion list)
15:30:43.97 +58:01:32.7 -- not an asteroid (will add it to exclusion list)
15:30:28.33 +58:06:25.7 -- not an asteroid (will add it to exclusion list)
15:26:10.02 +58:21:45.0 -- not an asteroid (will add it to exclusion list)
15:29:21.85 +58:02:11.4 -- not an asteroid (will add it to exclusion list)
15:26:54.72 +58:24:50.8 -- not an asteroid (will add it to exclusion list)
15:31:01.01 +57:47:12.1 -- not an asteroid (will add it to exclusion list)
15:34:23.07 +57:51:26.7 -- not an asteroid (will add it to exclusion list)
15:15:02.43 +61:25:20.5 -- not an asteroid (will add it to exclusion list)
15:29:13.65 +58:01:40.7 -- not an asteroid (will add it to exclusion list)
15:31:19.51 +58:01:04.5 -- not an asteroid (will add it to exclusion list)
15:33:12.08 +57:44:22.8 -- not an asteroid (will add it to exclusion list)
15:29:58.14 +57:55:47.2 -- not an asteroid (will add it to exclusion list)
15:29:53.65 +57:49:15.1 -- not an asteroid (will add it to exclusion list)
15:28:46.22 +58:00:43.4 -- not an asteroid (will add it to exclusion list)
15:29:44.94 +57:50:06.0 -- not an asteroid (will add it to exclusion list)
15:27:30.97 +58:11:41.7 -- not an asteroid (will add it to exclusion list)
15:31:18.25 +57:57:46.2 -- not an asteroid (will add it to exclusion list)
15:31:08.90 +58:07:10.6 -- not an asteroid (will add it to exclusion list)
15:26:20.38 +58:08:45.4 -- not an asteroid (will add it to exclusion list)
15:29:55.55 +57:54:09.2 -- not an asteroid (will add it to exclusion list)
15:27:39.76 +58:06:07.6 -- not an asteroid (will add it to exclusion list)
15:32:12.47 +57:45:53.4 -- not an asteroid (will add it to exclusion list)
15:32:01.20 +57:47:50.0 -- not an asteroid (will add it to exclusion list)
15:31:07.95 +57:46:01.5 -- not an asteroid (will add it to exclusion list)
15:27:01.09 +58:15:05.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
15:15:02.43 +61:25:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:16:47.45 +61:09:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:10.02 +58:21:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:20.38 +58:08:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:33.11 +58:07:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:54.72 +58:24:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:01.09 +58:15:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:30.97 +58:11:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:39.76 +58:06:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:25.23 +58:00:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:29.83 +58:00:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:34.42 +57:47:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:42.32 +58:12:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:46.22 +58:00:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:13.65 +58:01:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:21.85 +58:02:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:41.12 +58:06:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:44.94 +57:50:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:53.65 +57:49:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:53.90 +58:06:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:55.55 +57:54:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:58.14 +57:55:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:30:28.33 +58:06:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:30:43.97 +58:01:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:01.01 +57:47:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:02.00 +57:59:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:07.95 +57:46:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:08.90 +58:07:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:18.25 +57:57:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:19.51 +58:01:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:35.17 +57:58:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:54.24 +57:50:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:55.42 +57:52:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:32:01.20 +57:47:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:32:11.65 +57:46:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:32:12.47 +57:45:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:32:29.58 +58:05:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:33:12.08 +57:44:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:19.30 +57:53:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:23.07 +57:51:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:35:14.67 +57:56:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
15:15:02.43 +61:25:20.5 -- not a known variable star
15:16:47.45 +61:09:03.1 -- not a known variable star
15:26:10.02 +58:21:45.0 -- not a known variable star
15:26:20.38 +58:08:45.4 -- not a known variable star
15:26:33.11 +58:07:54.9 -- not a known variable star
15:26:54.72 +58:24:50.8 -- not a known variable star
15:27:01.09 +58:15:05.3 -- not a known variable star
15:27:30.97 +58:11:41.7 -- not a known variable star
15:27:39.76 +58:06:07.6 -- not a known variable star
15:28:25.23 +58:00:55.0 -- not a known variable star
15:28:29.83 +58:00:19.9 -- not a known variable star
15:28:34.42 +57:47:33.8 -- not a known variable star
15:28:42.32 +58:12:50.8 -- not a known variable star
15:28:46.22 +58:00:43.4 -- not a known variable star
15:29:13.65 +58:01:40.7 -- not a known variable star
15:29:21.85 +58:02:11.4 -- not a known variable star
15:29:41.12 +58:06:06.4 -- not a known variable star
15:29:44.94 +57:50:06.0 -- not a known variable star
15:29:53.65 +57:49:15.1 -- not a known variable star
15:29:53.90 +58:06:11.0 -- not a known variable star
15:29:55.55 +57:54:09.2 -- not a known variable star
15:29:58.14 +57:55:47.2 -- not a known variable star
15:30:28.33 +58:06:25.7 -- not a known variable star
15:30:43.97 +58:01:32.7 -- not a known variable star
15:31:01.01 +57:47:12.1 -- not a known variable star
15:31:02.00 +57:59:02.8 -- not a known variable star
15:31:07.95 +57:46:01.5 -- not a known variable star
15:31:08.90 +58:07:10.6 -- not a known variable star
15:31:18.25 +57:57:46.2 -- not a known variable star
15:31:19.51 +58:01:04.5 -- not a known variable star
15:31:35.17 +57:58:50.0 -- not a known variable star
15:31:54.24 +57:50:46.8 -- not a known variable star
15:31:55.42 +57:52:42.5 -- not a known variable star
15:32:01.20 +57:47:50.0 -- not a known variable star
15:32:11.65 +57:46:41.0 -- not a known variable star
15:32:12.47 +57:45:53.4 -- not a known variable star
15:32:29.58 +58:05:50.8 -- not a known variable star
15:33:12.08 +57:44:22.8 -- not a known variable star
15:34:19.30 +57:53:16.0 -- not a known variable star
15:34:23.07 +57:51:26.7 -- not a known variable star
15:35:14.67 +57:56:07.5 -- not a known variable star
Found 41 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
41 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 41 (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)2461245.86892000 -observatory V36
07:07:14.39 +18:32:12.6 Mercury (1.9mag)
11:08:01.95 +06:11:53.0 Venus (-4.2mag)
05:05:41.41 +22:50:22.6 Mars (1.3mag)
08:29:27.46 +19:29:26.9 Jupiter (-1.8mag)
00:56:46.85 +03:22:04.0 Saturn (0.7mag)
04:09:41.65 +20:51:37.6 Uranus (5.8mag)
00:16:46.16 +00:18:14.6 Neptune (7.7mag)
20:29:34.98 -23:24:07.5 Pluto (14.4mag)
15:57:59.51 -26:22:29.3 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 362 Jul 24 06:06 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461245.86892000:
08:29:31.64 +19:29:12.0 Io (6.0mag)
08:29:26.50 +19:29:32.3 Europa (6.3mag)
08:29:42.40 +19:28:29.4 Ganymede (5.6mag)
08:29:51.10 +19:27:56.6 Callisto (6.7mag)
08:27:24.52 +19:20:16.3 Himalia (15.7mag)
08:29:26.01 +19:29:33.8 Thebe (16.6mag)
08:26:47.50 +19:21:45.1 Elara (17.7mag)
08:33:21.71 +19:16:14.3 Pasiphae (17.9mag)
08:33:35.44 +19:36:46.4 Carme (19.0mag)
00:56:34.62 +03:22:15.7 Titan (8.5mag)
00:56:42.25 +03:21:56.8 Rhea (9.8mag)
00:56:18.47 +03:19:25.4 Iapetus (11.2mag)
00:56:54.77 +03:21:24.5 Hyperion (14.5mag)
00:56:28.81 +03:17:16.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 24 06:06 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461245.86892000:
18:12:47.48 -29:12:06.2 JWST
17:47:34.66 +33:15:36.3 Chandra
05:18:10.75 +43:57:27.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 24 06:06 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461245.86892000 -observatory V36
02:55:28.55 +15:59:23.8 17.8mag P/1996 R2 (Lagerkvist)
18:08:18.21 -34:37:13.6 13.8mag P/2010 H2 (Vales)
06:39:34.75 -68:25:50.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:05:29.19 +32:41:49.4 17.7mag C/2017 K2 (PANSTARRS)
02:53:36.69 +28:00:35.0 16.1mag P/2021 N1 (ZTF)
22:50:14.08 +32:05:44.5 17.3mag C/2022 E2 (ATLAS)
06:28:01.55 +26:46:15.5 16.7mag C/2022 N2 (PANSTARRS)
10:07:57.64 +29:08:44.3 16.9mag C/2022 QE78 (ATLAS)
09:18:55.41 +05:12:28.0 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.05 -11:45:48.6 17.8mag P/2023 B1 (PANSTARRS)
21:31:03.70 +67:13:47.6 17.9mag C/2023 H5 (Lemmon)
16:06:22.41 -11:30:31.8 14.1mag C/2023 R1 (PANSTARRS)
08:25:47.60 +66:30:54.2 18.0mag C/2024 A1 (ATLAS)
07:50:38.17 +30:40:42.1 15.0mag C/2024 E1 (Wierzchos)
15:10:35.08 +15:34:39.5 17.6mag C/2024 G6 (ATLAS)
19:22:46.86 +41:42:01.7 13.7mag C/2024 J3 (ATLAS)
21:31:22.67 +47:53:12.2 17.7mag C/2024 R4 (PANSTARRS)
05:02:32.18 -13:16:12.9 15.6mag C/2024 T5 (ATLAS)
06:45:44.29 +26:43:05.0 17.9mag C/2025 J1 (Borisov)
07:23:21.26 -14:17:05.0 17.2mag C/2025 R3 (PANSTARRS)
10:13:06.67 +21:46:07.1 17.5mag C/2025 V2 (Rankin)
12:50:11.64 +03:15:17.9 17.0mag C/2025 Y1 (ATLAS)
16:18:14.10 +78:55:08.7 17.1mag C/2026 A2 (Bok)
02:59:08.56 +45:47:04.8 16.9mag C/2026 B2 (Sun-Gao)
11:35:09.01 +06:45:08.7 17.1mag A/2026 E1
21:39:50.10 -20:44:12.5 6.9mag 10P/Tempel
11:20:30.05 -02:33:03.8 16.2mag 29P/Schwassmann-Wachmann
04:19:53.49 +31:01:14.5 17.9mag 47P/Ashbrook-Jackson
10:37:12.78 +09:29:46.8 17.1mag 63P/Wild
00:53:01.01 -05:05:10.9 15.5mag 65P/Gunn
05:01:01.51 +20:41:16.3 13.7mag 78P/Gehrels
02:43:17.82 +12:20:34.5 16.5mag 88P/Howell
07:16:07.26 +29:25:30.2 15.9mag 93P/Lovas
05:07:05.99 +31:16:33.9 16.6mag 114P/Wiseman-Skiff
08:42:51.20 +28:57:06.7 15.1mag 123P/West-Hartley
11:14:38.78 -04:27:29.2 16.9mag 124P/Mrkos
05:13:58.23 +21:06:43.0 16.2mag 128P/Shoemaker-Holt
06:02:16.42 +19:28:14.5 17.8mag 131P/Mueller
08:01:46.03 +13:50:04.0 17.2mag 141P-D/Machholz
03:21:45.88 -20:21:57.9 14.8mag 161P/Hartley-IRAS
06:23:37.69 +36:25:41.3 15.6mag 162P/SidingSpring
18:08:44.22 +25:49:05.1 13.5mag 169P/NEAT
02:13:09.05 +08:53:13.9 17.6mag 220P/McNaught
16:36:15.86 -09:05:15.9 17.3mag 235P/LINEAR
20:33:34.93 -52:02:16.5 17.8mag 259P/Garradd
02:39:02.15 +18:36:18.6 15.5mag 260P/McNaught
06:20:03.44 +37:38:53.8 17.3mag 295P/LINEAR
15:07:05.98 +04:43:10.4 17.6mag 391P/Kowalski
08:47:18.42 +19:04:37.3 17.9mag 450P/LONEOS
08:13:29.87 +38:01:49.9 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.4K Jul 24 06:06 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
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-26eg 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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -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
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
-rw-r--r-- 1 apache apache 5.6K Jul 24 06:06 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
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
-rw-r--r-- 1 apache apache 189K Jul 24 06:06 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:37:09.408 +59:50:34.02 AT 2026txe 2026-07-04.24 20.7267
15:28:44.304 +66:51:28.10 AT 2026txd 2026-07-08.26 20.2643
21:50:49.233 +24:57:52.83 AT 2026txc 2026-07-11.01 19.66
16:24:15.363 +53:52:26.55 AT 2026txb 2026-07-11.76 19.17
17:27:12.795 +25:29:25.90 AT 2026txa 2026-07-11.77 18.88
17:41:19.739 +49:31:59.41 AT 2026twz 2026-07-11.86 19.2
17:57:43.660 +27:18:37.46 AT 2026twy 2026-07-10.78 17.85
21:22:12.202 -05:27:50.11 AT 2026twx 2026-07-11.92 19.62
21:41:05.874 -00:44:05.29 AT 2026tww 2026-07-11.91 18.97
22:52:20.244 +08:14:57.79 AT 2026twv 2026-07-11.97 19.33
22:42:29.978 +07:49:23.31 AT 2026twu 2026-07-12.04 19.6
16:30:23.785 +54:01:13.69 AT 2026twt 2026-07-11.90 19.1
22:10:51.145 +08:26:42.80 AT 2026tws 2026-07-12.06 19.01
23:46:37.559 +04:51:10.62 AT 2026twr 2026-07-12.05 19.48
17:54:33.311 +44:32:29.77 AT 2026twq 2026-07-12.01 18.2
23:51:04.058 +06:06:30.13 AT 2026twp 2026-07-12.05 19.41
22:49:13.425 +07:24:01.48 AT 2026two 2026-07-12.03 19.46
22:00:35.405 +06:42:17.09 AT 2026twn 2026-07-12.05 19.07
17:03:26.927 +50:27:33.03 AT 2026twm 2026-07-10.92 19.51
23:54:42.693 +05:22:53.70 AT 2026twl 2026-07-12.05 19.64
-rw-r--r-- 1 apache apache 88K Jul 24 06:06 tns_transients_list.txt
