This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG
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 18.2608 2461239.7608 13.71 19:01:00.92 +73:28:07.7
104.61224 25.24921 galactic Dra Second-epoch detections are separated by 8.7" and 0.4 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 | 19:01:00.92 +73:28:07.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:01:00.92 +73:28:07.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:01:00.92 +73:28:07.7: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7608,13.71,0.05,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 20260718.2608 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 18.2608 2461239.7608 12.99 18:17:00.69 +67:59:47.9
98.07430 28.20778 galactic Dra Second-epoch detections are separated by 3.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:17:00.69 +67:59:47.9 (user input) | T | P | (position from user input) J-Ks=0.672+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:17:00.69 +67:59:47.9: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:17:00.69 +67:59:47.9: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461239.7608,12.99,0.05,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 20260718.2608 12.99CV 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 18.2608 2461239.7608 13.01 18:00:52.12 +68:14:54.3
98.32745 29.71605 galactic Dra Second-epoch detections are separated by 0.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:00:52.12 +68:14:54.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:00:52.12 +68:14:54.3: 13.96 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:00:52.12 +68:14:54.3: 13.96 +/- 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,2461239.7608,13.01,0.05,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 20260718.2608 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.18 19:00:00.02 +74:09:19.1
105.34577 25.44107 galactic Dra Second-epoch detections are separated by 1.7" and 1.7 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 | 19:00:00.02 +74:09:19.1 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.038 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:00:00.02 +74:09:19.1: 14.17 +/- 0.07 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:00:00.02 +74:09:19.1: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461239.7608,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.71 18:19:31.62 +68:26:59.0
98.60210 28.00052 galactic Dra Second-epoch detections are separated by 2.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:19:31.62 +68:26:59.0 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.035 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:19:31.62 +68:26:59.0: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:19:31.62 +68:26:59.0: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7608,12.71,0.05,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 20260718.2608 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 18.2608 2461239.7608 12.81 19:59:06.43 +68:18:48.1
100.95432 19.14793 galactic Dra Second-epoch detections are separated by 0.4" and 1.7 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 | 19:59:06.43 +68:18:48.1 (user input) | T | P | (position from user input) J-Ks=0.628+/-0.031 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:06.43 +68:18:48.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:06.43 +68:18:48.1: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461239.7608,12.81,0.05,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 20260718.2608 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 18.2608 2461239.7608 12.09 19:59:35.99 +68:10:58.1
100.85085 19.05012 galactic Dra Second-epoch detections are separated by 1.4" and 1.8 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 | 19:59:35.99 +68:10:58.1 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.036 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:35.99 +68:10:58.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:35.99 +68:10:58.1: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461239.7608,12.09,0.05,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 20260718.2608 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.41 19:59:47.45 +68:17:17.7
100.95943 19.08010 galactic Dra Second-epoch detections are separated by 1.2" and 2.0 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 | 19:59:47.45 +68:17:17.7 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.030 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:47.45 +68:17:17.7: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:47.45 +68:17:17.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461239.7608,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.49 19:54:13.35 +67:02:01.5
99.52053 19.01969 galactic Dra Second-epoch detections are separated by 0.6" and 2.0 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 | 19:54:13.35 +67:02:01.5 (user input) | T | P | (position from user input) J-Ks=0.735+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:54:13.35 +67:02:01.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:54:13.35 +67:02:01.5: 13.39 +/- 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,2461239.7608,12.49,0.05,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 20260718.2608 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 18.2608 2461239.7608 12.86 19:58:21.62 +68:22:24.6
100.98027 19.23604 galactic Dra Second-epoch detections are separated by 1.2" and 2.0 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 | 19:58:21.62 +68:22:24.6 (user input) | T | P | (position from user input) J-Ks=0.724+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:58:21.62 +68:22:24.6: 13.94 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:58:21.62 +68:22:24.6: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461239.7608,12.86,0.05,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 20260718.2608 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 18.2608 2461239.7608 12.97 18:00:25.60 +68:24:08.1
98.50531 29.75448 galactic Dra Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:00:25.60 +68:24:08.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:00:25.60 +68:24:08.1: 13.94 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:00:25.60 +68:24:08.1: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461239.7608,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.01 18:13:41.92 +68:35:10.2
98.72821 28.53995 galactic Dra Second-epoch detections are separated by 1.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:13:41.92 +68:35:10.2 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.033 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:13:41.92 +68:35:10.2: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:13:41.92 +68:35:10.2: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461239.7608,13.01,0.05,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 20260718.2608 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.01 18:24:56.54 +69:03:40.3
99.32906 27.55242 galactic Dra Second-epoch detections are separated by 1.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:24:56.54 +69:03:40.3 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.031 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:56.54 +69:03:40.3: 13.96 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:56.54 +69:03:40.3: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461239.7608,13.01,0.05,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 20260718.2608 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.02 18:10:50.63 +68:41:09.8
98.83352 28.80270 galactic Dra Second-epoch detections are separated by 0.6" and 2.0 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 | 18:10:50.63 +68:41:09.8 (user input) | T | P | (position from user input) J-Ks=0.634+/-0.029 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:10:50.63 +68:41:09.8: 13.94 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:10:50.63 +68:41:09.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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,2461239.7608,13.02,0.05,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 20260718.2608 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 18.2608 2461239.7608 12.76 18:11:38.58 +68:15:18.5
98.34431 28.71816 galactic Dra Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:11:38.58 +68:15:18.5 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.031 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:11:38.58 +68:15:18.5: 13.57 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:11:38.58 +68:15:18.5: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461239.7608,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.13 18:12:20.11 +68:04:42.3
98.14532 28.64818 galactic Dra Second-epoch detections are separated by 2.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:12:20.11 +68:04:42.3 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.037 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:12:20.11 +68:04:42.3: 14.09 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:12:20.11 +68:04:42.3: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461239.7608,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.91 18:27:43.07 +69:02:50.6
99.33627 27.30408 galactic Dra Second-epoch detections are separated by 1.0" and 2.0 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 | 18:27:43.07 +69:02:50.6 (user input) | T | P | (position from user input) J-Ks=-0.056+/-0.052 (B)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:27:43.07 +69:02:50.6: 13.91 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:27:43.07 +69:02:50.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7608,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.13 19:59:33.91 +68:13:06.5
100.88334 19.06854 galactic Dra Second-epoch detections are separated by 1.1" and 2.0 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 | 19:59:33.91 +68:13:06.5 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.035 (F)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:33.91 +68:13:06.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:33.91 +68:13:06.5: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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,2461239.7608,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.08 18:24:53.86 +69:15:06.5
99.54314 27.57063 galactic Dra Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:24:53.86 +69:15:06.5 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:53.86 +69:15:06.5: 14.20 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:53.86 +69:15:06.5: 14.05 +/- 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,2461239.7608,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.09 18:29:14.29 +67:46:23.9
97.92569 27.04312 galactic Dra Second-epoch detections are separated by 1.5" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:29:14.29 +67:46:23.9 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.047 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:14.29 +67:46:23.9: 14.26 +/- 0.07 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:14.29 +67:46:23.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461239.7608,13.09,0.05,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 20260718.2608 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.96 18:33:01.55 +68:01:26.4
98.24917 26.71674 galactic Dra Second-epoch detections are separated by 1.0" and 2.0 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 | 18:33:01.55 +68:01:26.4 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.034 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:33:01.55 +68:01:26.4: 13.89 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:33:01.55 +68:01:26.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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,2461239.7608,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.83 18:26:20.10 +69:11:57.3
99.49511 27.43951 galactic Dra Second-epoch detections are separated by 0.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:26:20.10 +69:11:57.3 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.035 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:26:20.10 +69:11:57.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:26:20.10 +69:11:57.3: 13.80 +/- 0.05 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,2461239.7608,12.83,0.05,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
target 20260718.2608 12.83CV 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 18.2608 2461239.7608 12.80 19:59:21.79 +68:23:25.5
101.03867 19.16004 galactic Dra Second-epoch detections are separated by 0.2" and 1.8 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 | 19:59:21.79 +68:23:25.5 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.030 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:21.79 +68:23:25.5: 13.74 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:21.79 +68:23:25.5: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461239.7608,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.93 19:11:30.81 +68:14:09.5
99.22959 23.24174 galactic Dra Second-epoch detections are separated by 2.6" and 2.3 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 | 19:11:30.81 +68:14:09.5 (user input) | T | P | (position from user input) J-Ks=0.228+/-0.042 (F)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:11:30.81 +68:14:09.5: 14.05 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:11:30.81 +68:14:09.5: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461239.7608,12.93,0.05,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 20260718.2608 12.93CV 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 18.2608 2461239.7608 12.89 18:29:25.77 +67:50:40.4
98.00736 27.03258 galactic Dra Second-epoch detections are separated by 3.4" and 1.8 pix
The object was found in VSX 2" Gaia DR3 2258916716230347136
Type: ROT
# Max. Min./Amp. JD0 Period
13.760 G 13.800 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:25.77 +67:50:40.4: 13.86 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:25.77 +67:50:40.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2258916716230347136,2461239.7608,12.89,0.05,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 2258916716230347136 20260718.2608 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.73 18:27:08.04 +67:57:25.4
98.10907 27.25858 galactic Dra Second-epoch detections are separated by 1.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:27:08.04 +67:57:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:27:08.04 +67:57:25.4: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:27:08.04 +67:57:25.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461239.7608,12.73,0.05,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 20260718.2608 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 18.2608 2461239.7608 12.84 19:59:46.61 +68:20:33.8
101.01073 19.10498 galactic Dra Second-epoch detections are separated by 1.4" and 1.5 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 | 19:59:46.61 +68:20:33.8 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.149 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:46.61 +68:20:33.8: 14.02 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:46.61 +68:20:33.8: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461239.7608,12.84,0.05,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
target 20260718.2608 12.84CV 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 18.2608 2461239.7608 12.54 19:12:57.09 +68:10:42.4
99.20781 23.09779 galactic Dra Second-epoch detections are separated by 0.9" and 2.0 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 | 19:12:57.09 +68:10:42.4 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.029 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:12:57.09 +68:10:42.4: 13.49 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:12:57.09 +68:10:42.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461239.7608,12.54,0.05,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 20260718.2608 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 18.2608 2461239.7608 12.87 18:20:32.17 +68:10:13.2
98.29309 27.88989 galactic Dra Second-epoch detections are separated by 0.1" and 2.0 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 | 18:20:32.17 +68:10:13.2 (user input) | T | P | (position from user input) J-Ks=0.846+/-0.031 (M)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:20:32.17 +68:10:13.2: 13.84 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:20:32.17 +68:10:13.2: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461239.7608,12.87,0.05,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 20260718.2608 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 18.2608 2461239.7608 12.80 18:25:22.98 +68:01:13.2
98.16329 27.42770 galactic Dra Second-epoch detections are separated by 1.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:25:22.98 +68:01:13.2 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.036 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:25:22.98 +68:01:13.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:25:22.98 +68:01:13.2: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461239.7608,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.79 17:59:42.75 +68:20:14.0
98.43178 29.82147 galactic Dra Second-epoch detections are separated by 1.7" and 2.3 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 | Large-amplitude variable Gaia DR2 1634502791504960000 | 17:59:42.75 +68:20:14.0 (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=0.321+/-0.038 (F)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 17:59:42.75 +68:20:14.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 17:59:42.75 +68:20:14.0: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1634502791504960000,2461239.7608,12.79,0.05,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
Large-amplitude variable Gaia DR2 1634502791504960000 20260718.2608 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 18.2608 2461239.7608 10.96 19:52:56.95 +67:35:21.9
100.00024 19.36406 galactic Dra Second-epoch detections are separated by 0.4" and 1.8 pix
The object was found in VSX 3" NSVS J1952574+673522
Type: SR
# Max. Min./Amp. JD0 Period
13.370 g Y 0.503 g 2458655.76080 122.662379300000
The object was not found in astcheck.
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:52:56.95 +67:35:21.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:52:56.95 +67:35:21.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1952574+673522,2461239.7608,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1952574+673522 20260718.2608 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.91 18:15:47.95 +68:37:03.5
98.77247 28.34974 galactic Dra Second-epoch detections are separated by 1.1" and 2.0 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 | 18:15:47.95 +68:37:03.5 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:15:47.95 +68:37:03.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:15:47.95 +68:37:03.5: 13.82 +/- 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,2461239.7608,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.12 18:24:20.36 +69:18:31.7
99.60326 27.62400 galactic Dra Second-epoch detections are separated by 1.1" and 2.0 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 | 18:24:20.36 +69:18:31.7 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.033 (K)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:20.36 +69:18:31.7: 14.08 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:20.36 +69:18:31.7: 14.11 +/- 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,2461239.7608,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.92 18:24:28.37 +69:18:14.8
99.59892 27.61191 galactic Dra Second-epoch detections are separated by 4.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:24:28.37 +69:18:14.8 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.035 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:28.37 +69:18:14.8: 13.79 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:28.37 +69:18:14.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461239.7608,12.92,0.05,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 20260718.2608 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 18.2608 2461239.7608 13.14 18:29:05.60 +67:42:17.8
97.84775 27.04964 galactic Dra Second-epoch detections are separated by 1.5" and 2.3 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 | 18:29:05.60 +67:42:17.8 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.038 (G)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:05.60 +67:42:17.8: 14.12 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:05.60 +67:42:17.8: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461239.7608,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2608 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 13.11 18:52:55.45 +73:42:20.2
104.76613 25.85205 galactic Dra Second-epoch detections are separated by 0.4" and 1.6 pix
The object was found in VSX 2" NSVS 1203522
Type: SR
# Max. Min./Amp. JD0 Period
15.585 g Y 0.630 g 2451613.38000 145.504517000000
The object was not found in astcheck.
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:52:55.45 +73:42:20.2: 14.20 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:52:55.45 +73:42:20.2: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1203522,2461239.7608,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1203522 20260718.2608 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2608 2461239.7608 12.74 18:21:40.56 +68:15:50.6
98.40697 27.79076 galactic Dra Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:21:40.56 +68:15:50.6 (user input) | T | P | (position from user input) J-Ks=0.250+/-0.034 (F)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:21:40.56 +68:15:50.6: 13.60 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:21:40.56 +68:15:50.6: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461239.7608,12.74,0.05,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 20260718.2608 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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: 2461202.84134294 11.06.2026 08:11:22.030 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
First image: 2461202.84134294 11.06.2026 08:11:22.030 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Last image: 2461239.76106830 18.07.2026 06:15:46.301 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
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: 8 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): 11045
Objects passed selection criteria: 10989
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 7534.5
Average stars matched: 7337.5 (97.3854 %)
Memory usage VmPeak: 120772 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:27:13 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: 2461202.84134294 11.06.2026 08:11:22.030 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
First image: 2461202.84134294 11.06.2026 08:11:22.030 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Last image: 2461239.76106830 18.07.2026 06:15:46.301 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 243
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.08
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: 71 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): 67151
Objects passed selection criteria: 66969
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 48285.2
Average stars matched: 46721.5 (96.7614 %)
Memory usage VmPeak: 174284 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:31:59 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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.cat to cache
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461239.76061087
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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits exists and is non-empty
Saving wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits to local_wcs_cache/
'wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits' -> 'local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits'
wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits exists and is non-empty
Saving wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits to local_wcs_cache/
'wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits' -> 'local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits'
wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits exists and is non-empty
Saving wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits to local_wcs_cache/
'wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits'
wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits (1st reference image)
verification OK: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:12:05.078 +70:01:39.07 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-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits (1st new image)
verification OK: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Image size: 936.9'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: 19:11:59.704 +70:02:02.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:12:05.078 +70:01:39.07
Second-epoch image center 19:11:59.704 +70:02:02.66
Angular distance between the image centers 0.0101 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits (2nd new image)
verification OK: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Image size: 936.9'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: 19:11:57.702 +70:02:05.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:12:05.078 +70:01:39.07
Second-epoch image center 19:11:57.702 +70:02:05.36
Angular distance between the image centers 0.0128 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 19:11:59.704 +70:02:02.66
Second-epoch second image center 19:11:57.702 +70:02:05.36
Angular distance between the image centers 0.00295 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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits &> /tmp/tmp.nGhQK1sD9X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits &> /tmp/tmp.Ms9SNjIk2d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits &> /tmp/tmp.6dFk0RVqLh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits &> /tmp/tmp.Li4A627JB8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
Found non-empty wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
The reference image (wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits) and catalog (wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat) found
'wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat' -> 'wcsmag.cat'
Read 15402 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 260.2567 to 316.2860 deg, Dec +63.6438 to +75.2941 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 260.2567 to 316.2860 deg, Dec 63.6438 to 75.2941 deg
Loaded 13053 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): 7912 out of 8266 total matches.
Matched with Tycho-2 8266 out of 15402 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.691200
a=0.000000 b=1.000000 c=22.691200
From vast_summary.log: estimated ref. image limiting mag.: -7.40
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 15402 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 260.2567 to 316.2860 deg, Dec +63.6438 to +75.2941 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 260.2567 to 316.2860 deg, Dec 63.6438 to 75.2941 deg
Loaded 13053 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): 7912 out of 8266 total matches.
Matched with Tycho-2 8266 out of 15402 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits:
Forced-photometry filter: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits -> calib.txt_param_ref_wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits (aperture=6.1)
Read 15513 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 260.2573 to 316.2876 deg, Dec +63.6437 to +75.2969 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 260.2573 to 316.2876 deg, Dec 63.6437 to 75.2969 deg
Loaded 13056 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): 7917 out of 8279 total matches.
Matched with Tycho-2 8279 out of 15513 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits:
Forced-photometry filter: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits -> calib.txt_param_ref_wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
2.2 pix Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
2.5 pix fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
2.5 pix fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
2.2 pix wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
2.2 pix wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Limiting magnitude estimates:
15.3 mag. Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
15.3 mag. Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
13.3 mag. fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
13.1 mag. fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.9 (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.nGhQK1sD9X (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits' -> 'wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=889, bad_region=3680, passed=15395
Got 15395 stars (including 10990 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
util/solve_plate_with_UCAC5 got 15395 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 768 to 828 (Dec 63.6 to 75.3)
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(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12006 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 768 to 828 (Dec 63.6 to 75.3)
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(), 12007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits N_match=970 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.497 n_q1=294 n_q2=215 n_q3=262 n_q4=199 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits -region wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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.Ms9SNjIk2d (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits' -> 'wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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=885, bad_region=3629, passed=15513
Got 15513 stars (including 11153 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 15513 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 768 to 828 (Dec 63.6 to 75.3)
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(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 12129 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 768 to 828 (Dec 63.6 to 75.3)
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(), 12128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 12128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits N_match=968 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.479 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.505 n_q1=297 n_q2=208 n_q3=268 n_q4=195 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits -region wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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.6dFk0RVqLh (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=153, bad_region=965, passed=4311
Got 4311 stars (including 3226 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 4311 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 768 to 828 (Dec 63.8 to 75.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.8 to 75.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3394 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits N_match=961 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.618 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.561 n_q1=270 n_q2=155 n_q3=362 n_q4=174 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits -region wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Li4A627JB8 (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=141, bad_region=930, passed=4290
Got 4290 stars (including 3250 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 4290 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 768 to 828 (Dec 63.8 to 75.3)
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: 968 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.8 to 75.3)
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: 967 matched stars entering correct_measured_positions(), 3436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits N_match=967 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.554 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.652 n_q1=273 n_q2=166 n_q3=356 n_q4=172 worst_quadrant_to_overall_ratio=1.376
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits -region wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits sigma_overall=0.447 worst_q_ratio=1.135
ref2=Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits sigma_overall=0.425 worst_q_ratio=1.187
new1=fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits sigma_overall=0.456 worst_q_ratio=1.355
new2=fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits sigma_overall=0.474 worst_q_ratio=1.376
reference average sigma_overall=0.436 worst_q_ratio=1.161
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238_astrometric_residuals.png (970 matched stars from wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239_astrometric_residuals.png (968 matched stars from wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226_astrometric_residuals.png (961 matched stars from wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227_astrometric_residuals.png (967 matched stars from wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.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-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits'
Preparing the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-05-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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.cat to cache
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Creating symlink local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits exists and is non-empty
wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits exists and is non-empty
wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits (1st reference image)
verification OK: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:12:05.078 +70:01:39.07 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-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits (1st new image)
verification OK: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Image size: 936.9'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: 19:11:59.704 +70:02:02.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:12:05.078 +70:01:39.07
Second-epoch image center 19:11:59.704 +70:02:02.66
Angular distance between the image centers 0.0101 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits (2nd new image)
verification OK: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Image size: 936.9'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: 19:11:57.702 +70:02:05.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:12:05.078 +70:01:39.07
Second-epoch image center 19:11:57.702 +70:02:05.36
Angular distance between the image centers 0.0128 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 19:11:59.704 +70:02:02.66
Second-epoch second image center 19:11:57.702 +70:02:05.36
Angular distance between the image centers 0.00295 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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits &> /tmp/tmp.ZnxrUqIopk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits &> /tmp/tmp.tIwlokiteq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits &> /tmp/tmp.AXFlUAHcMI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits &> /tmp/tmp.9rCdgN2wBh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
Found non-empty wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits and wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
The reference image (wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits) and catalog (wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat) found
'wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat' -> 'wcsmag.cat'
Read 87306 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 259.8695 to 316.2859 deg, Dec +63.5727 to +75.2954 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 259.8695 to 316.2859 deg, Dec 63.5727 to 75.2954 deg
Loaded 13259 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): 7220 out of 8380 total matches.
Matched with Tycho-2 8380 out of 87306 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.553300
a=0.000000 b=1.000000 c=22.553300
From vast_summary.log: estimated ref. image limiting mag.: -7.08
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 87306 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 259.8695 to 316.2859 deg, Dec +63.5727 to +75.2954 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 259.8695 to 316.2859 deg, Dec 63.5727 to 75.2954 deg
Loaded 13259 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): 7220 out of 8380 total matches.
Matched with Tycho-2 8380 out of 87306 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits:
Forced-photometry filter: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits -> calib.txt_param_ref_wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits (aperture=4.7)
Read 87167 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 259.8489 to 316.2875 deg, Dec +63.6396 to +75.3023 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 259.8489 to 316.2875 deg, Dec 63.6396 to 75.3023 deg
Loaded 13147 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): 7239 out of 8384 total matches.
Matched with Tycho-2 8384 out of 87167 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits:
Forced-photometry filter: calibrated wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits -> calib.txt_param_ref_wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 95 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
2.1 pix Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
2.4 pix fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
2.4 pix fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
2.1 pix wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
2.1 pix wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Limiting magnitude estimates:
15.5 mag. Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
15.5 mag. Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
13.7 mag. fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
13.6 mag. fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZnxrUqIopk (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits' -> 'wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=6474, bad_region=14130, passed=87289
Got 87289 stars (including 68116 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat
util/solve_plate_with_UCAC5 got 87289 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 767 to 828 (Dec 63.6 to 75.3)
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(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 74271 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 767 to 828 (Dec 63.6 to 75.3)
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(), 74270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 74270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits N_match=971 sigma_overall_arcsec=0.446 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.456 sigma_q3_arcsec=0.391 sigma_q4_arcsec=0.524 n_q1=297 n_q2=215 n_q3=277 n_q4=182 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits -region wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.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.tIwlokiteq (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits' -> 'wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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=10, blended=6408, bad_region=13846, passed=87157
Got 87157 stars (including 68236 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 87157 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 768 to 828 (Dec 63.6 to 75.3)
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(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 74385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 768 to 828 (Dec 63.6 to 75.3)
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(), 74385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 74385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits N_match=969 sigma_overall_arcsec=0.429 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.510 n_q1=299 n_q2=201 n_q3=279 n_q4=190 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits -region wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.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.AXFlUAHcMI (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1126, bad_region=4720, passed=28864
Got 28864 stars (including 23448 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 28864 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits N_match=960 sigma_overall_arcsec=0.471 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.612 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.571 n_q1=273 n_q2=146 n_q3=370 n_q4=171 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits -region wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9rCdgN2wBh (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_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1048, bad_region=4662, passed=28317
Got 28317 stars (including 23003 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 28317 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 23974 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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 23975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 23975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 966 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits N_match=966 sigma_overall_arcsec=0.486 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.571 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.603 n_q1=274 n_q2=162 n_q3=363 n_q4=167 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits -region wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-06_20.00sec_4.90C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Dra-05-Q2b1x1_013640_TTUQ2b1x1_1359768_YTsiecaG/wcs_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227.fits
Preparing the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:11:59.15 +66:09:11.3: 12.50 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:11:59.15 +66:09:11.3: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 18:11:59.15 +66:09:11.3: ref_mag=12.53 +/- 0.01 new_mean_mag=12.6424 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:01:00.92 +73:28:07.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:01:00.92 +73:28:07.7: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:17:00.69 +67:59:47.9: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:00:52.12 +68:14:54.3: 13.96 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:00:00.02 +74:09:19.1: 14.17 +/- 0.07 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:19:31.62 +68:26:59.0: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:06.43 +68:18:48.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:35.99 +68:10:58.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:00:52.12 +68:14:54.3: 13.96 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:17:00.69 +67:59:47.9: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry filter KEPT candidate at 18:17:00.69 +67:59:47.9: ref_mag=13.95 +/- 0.04 new_mean_mag=12.9543 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 18:00:52.12 +68:14:54.3: ref_mag=13.96 +/- 0.04 new_mean_mag=12.9794 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:00:00.02 +74:09:19.1: 14.13 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:19:31.62 +68:26:59.0: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Forced photometry filter KEPT candidate at 19:00:00.02 +74:09:19.1: ref_mag=14.15 +/- 0.05 new_mean_mag=13.1679 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 18:19:31.62 +68:26:59.0: ref_mag=13.65 +/- 0.03 new_mean_mag=12.6536 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:47.45 +68:17:17.7: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:06.43 +68:18:48.1: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:06.43 +68:18:48.1: ref_mag=13.72 +/- 0.03 new_mean_mag=12.8060 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:54:13.35 +67:02:01.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:35.99 +68:10:58.1: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:35.99 +68:10:58.1: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0845 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:58:21.62 +68:22:24.6: 13.94 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:47.45 +68:17:17.7: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:47.45 +68:17:17.7: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4040 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:54:13.35 +67:02:01.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 19:54:13.35 +67:02:01.5: ref_mag=13.38 +/- 0.02 new_mean_mag=12.4470 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:58:21.62 +68:22:24.6: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 19:58:21.62 +68:22:24.6: ref_mag=13.93 +/- 0.04 new_mean_mag=12.7967 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:00:25.60 +68:24:08.1: 13.94 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:13:41.92 +68:35:10.2: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:00:25.60 +68:24:08.1: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 18:00:25.60 +68:24:08.1: ref_mag=13.94 +/- 0.04 new_mean_mag=12.9440 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:13:41.92 +68:35:10.2: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 18:13:41.92 +68:35:10.2: ref_mag=13.94 +/- 0.04 new_mean_mag=12.9631 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:56.54 +69:03:40.3: 13.96 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:10:50.63 +68:41:09.8: 13.94 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:56.54 +69:03:40.3: 13.91 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:10:50.63 +68:41:09.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 18:24:56.54 +69:03:40.3: ref_mag=13.93 +/- 0.04 new_mean_mag=13.0016 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Forced photometry filter KEPT candidate at 18:10:50.63 +68:41:09.8: ref_mag=13.97 +/- 0.04 new_mean_mag=12.9544 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:11:38.58 +68:15:18.5: 13.57 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:12:20.11 +68:04:42.3: 14.09 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:33.91 +68:13:06.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:27:43.07 +69:02:50.6: 13.91 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:11:38.58 +68:15:18.5: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 18:11:38.58 +68:15:18.5: ref_mag=13.64 +/- 0.03 new_mean_mag=12.7223 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:12:20.11 +68:04:42.3: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Forced photometry filter KEPT candidate at 18:12:20.11 +68:04:42.3: ref_mag=14.11 +/- 0.04 new_mean_mag=13.1361 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:33.91 +68:13:06.5: 13.07 +/- 0.02 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:27:43.07 +69:02:50.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:33.91 +68:13:06.5: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1189 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 18:27:43.07 +69:02:50.6: ref_mag=13.90 +/- 0.04 new_mean_mag=12.9132 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:53.86 +69:15:06.5: 14.20 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:53.86 +69:15:06.5: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 18:24:53.86 +69:15:06.5: ref_mag=14.12 +/- 0.04 new_mean_mag=13.0740 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:14.29 +67:46:23.9: 14.26 +/- 0.07 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:14.29 +67:46:23.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Forced photometry filter KEPT candidate at 18:29:14.29 +67:46:23.9: ref_mag=14.24 +/- 0.05 new_mean_mag=13.0459 delta=1.20 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:33:01.55 +68:01:26.4: 13.89 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:33:01.55 +68:01:26.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter KEPT candidate at 18:33:01.55 +68:01:26.4: ref_mag=13.87 +/- 0.03 new_mean_mag=12.9456 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:26:20.10 +69:11:57.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:26:20.10 +69:11:57.3: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 18:26:20.10 +69:11:57.3: ref_mag=13.78 +/- 0.03 new_mean_mag=12.8021 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:21.79 +68:23:25.5: 13.74 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:21.79 +68:23:25.5: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:21.79 +68:23:25.5: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7889 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:11:30.81 +68:14:09.5: 14.05 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:11:30.81 +68:14:09.5: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter KEPT candidate at 19:11:30.81 +68:14:09.5: ref_mag=14.00 +/- 0.04 new_mean_mag=12.9252 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:25.77 +67:50:40.4: 13.86 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:27:08.04 +67:57:25.4: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:59:46.61 +68:20:33.8: 14.02 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:25.77 +67:50:40.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 18:29:25.77 +67:50:40.4: ref_mag=13.86 +/- 0.03 new_mean_mag=12.8962 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:27:08.04 +67:57:25.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 18:27:08.04 +67:57:25.4: ref_mag=13.64 +/- 0.03 new_mean_mag=12.6746 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:59:46.61 +68:20:33.8: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry filter KEPT candidate at 19:59:46.61 +68:20:33.8: ref_mag=14.05 +/- 0.04 new_mean_mag=12.8287 delta=1.22 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:12:57.09 +68:10:42.4: 13.49 +/- 0.03 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:12:57.09 +68:10:42.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 19:12:57.09 +68:10:42.4: ref_mag=13.46 +/- 0.02 new_mean_mag=12.4858 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:20:32.17 +68:10:13.2: 13.84 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:20:32.17 +68:10:13.2: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter KEPT candidate at 18:20:32.17 +68:10:13.2: ref_mag=13.84 +/- 0.03 new_mean_mag=12.8691 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:25:22.98 +68:01:13.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 17:59:42.75 +68:20:14.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:25:22.98 +68:01:13.2: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 18:25:22.98 +68:01:13.2: ref_mag=13.83 +/- 0.03 new_mean_mag=12.7701 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 17:59:42.75 +68:20:14.0: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 17:59:42.75 +68:20:14.0: ref_mag=13.70 +/- 0.03 new_mean_mag=12.7817 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 19:52:56.95 +67:35:21.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 19:52:56.95 +67:35:21.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter KEPT candidate at 19:52:56.95 +67:35:21.9: ref_mag=12.17 +/- 0.01 new_mean_mag=10.9117 delta=1.25 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:15:47.95 +68:37:03.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:15:47.95 +68:37:03.5: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter KEPT candidate at 18:15:47.95 +68:37:03.5: ref_mag=13.82 +/- 0.03 new_mean_mag=12.8808 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:20.36 +69:18:31.7: 14.08 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:24:28.37 +69:18:14.8: 13.79 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:20.36 +69:18:31.7: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry filter KEPT candidate at 18:24:20.36 +69:18:31.7: ref_mag=14.09 +/- 0.04 new_mean_mag=13.1176 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:24:28.37 +69:18:14.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 18:24:28.37 +69:18:14.8: ref_mag=13.83 +/- 0.03 new_mean_mag=12.9025 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:29:05.60 +67:42:17.8: 14.12 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:29:05.60 +67:42:17.8: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Forced photometry filter KEPT candidate at 18:29:05.60 +67:42:17.8: ref_mag=14.19 +/- 0.05 new_mean_mag=13.1430 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:52:55.45 +73:42:20.2: 14.20 +/- 0.06 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:52:55.45 +73:42:20.2: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.05
Forced photometry filter KEPT candidate at 18:52:55.45 +73:42:20.2: ref_mag=14.20 +/- 0.05 new_mean_mag=13.1003 delta=1.10 (need > 0.90)
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-11-22_20.00sec_4.90C_LIGHT_0238.fits at 18:21:40.56 +68:15:50.6: 13.60 +/- 0.04 detection
Forced photometry on wcs_Dra-05-Q2b1x1_2026-06-11_03-12-00_20.00sec_5.00C_LIGHT_0239.fits at 18:21:40.56 +68:15:50.6: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 18:21:40.56 +68:15:50.6: ref_mag=13.64 +/- 0.03 new_mean_mag=12.7155 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out103462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66812.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 67s
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: 24s
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Considering the candidate 103328_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103328_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 103329_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103329_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 103331_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103331_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103332_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103332_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 103340_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103340_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 103346_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103346_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 103347_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103347_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 18:15:11.48 +68:43:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103348_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103348_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 103351_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103351_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 103352_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103352_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 20:05:22.02 +73:26:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103356_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103356_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 19:12:06.49 +67:40:34.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 103357_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103357_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 103364_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103364_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 103365_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103365_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 103366_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103366_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 103369_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103369_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 103375_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103375_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 103380_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103380_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 103381_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103381_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 103387_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103387_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 103392_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103392_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 103394_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103394_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 103395_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103395_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 103396_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103396_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 103397_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103397_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 103404_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103404_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 103408_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103408_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 103409_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103409_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 103411_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103411_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 103412_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103412_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 103413_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103413_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
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Considering the candidate 103414_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103414_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 103415_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103415_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 103417_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103417_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 103418_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103418_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 103422_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103422_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103425_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103425_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 103427_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103427_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 103428_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103428_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 103429_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103429_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 103432_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103432_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 103435_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103435_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 103449_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103449_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 103458_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103458_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 103462_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 103462_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 103463_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103463_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 103466_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103466_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 103474_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103474_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 103480_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 103480_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 33770_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 33770_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 39338_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 39338_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 24049_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 24049_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 19:12:33.65 +67:39:47.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 62995_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 62995_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 37473_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37473_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 66476_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 66476_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 37060_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37060_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 35910_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 35910_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 36924_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 36924_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 24508_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 24508_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 37448_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37448_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 40788_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 40788_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 39712_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 39712_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 42199_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 42199_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 41111_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 41111_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 65093_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 65093_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
**** FOUND 20:02:50.36 +73:27:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14305_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 14305_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 37119_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37119_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 35458_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 35458_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 41658_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 41658_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 36221_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 36221_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 43891_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 43891_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 29862_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 29862_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 31643_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 31643_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 52182_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 52182_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 43221_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 43221_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 37803_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37803_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 31679_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 31679_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 43560_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 43560_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 30526_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 30526_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 31793_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 31793_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
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Considering the candidate 37419_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 37419_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44265_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 44265_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31148_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 31148_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34800_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 34800_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83812_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 83812_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43351_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
The candidate 43351_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32681_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 32681_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40377_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 40377_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29245_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 29245_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39622_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 39622_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44453_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 44453_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44348_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 44348_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29265_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 29265_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66812_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 66812_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35490_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
Preparing report for the candidate 35490_fd_Dra-05-Q2b1x1_2026-07-18_01-15-46_20.00sec_5.00C_LIGHT_0227
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 94s
Prepared the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:01:00.92 +73:28:07.7
19:54:13.35 +67:02:01.5
19:52:56.95 +67:35:21.9
18:29:05.60 +67:42:17.8
18:29:14.29 +67:46:23.9
18:29:25.77 +67:50:40.4
19:12:57.09 +68:10:42.4
18:33:01.55 +68:01:26.4
19:11:30.81 +68:14:09.5
18:27:08.04 +67:57:25.4
18:25:22.98 +68:01:13.2
18:17:00.69 +67:59:47.9
18:20:32.17 +68:10:13.2
18:12:20.11 +68:04:42.3
18:21:40.56 +68:15:50.6
19:59:35.99 +68:10:58.1
19:59:33.91 +68:13:06.5
19:59:47.45 +68:17:17.7
19:59:06.43 +68:18:48.1
18:11:38.58 +68:15:18.5
19:59:46.61 +68:20:33.8
19:58:21.62 +68:22:24.6
18:19:31.62 +68:26:59.0
19:59:21.79 +68:23:25.5
18:00:52.12 +68:14:54.3
18:15:47.95 +68:37:03.5
18:13:41.92 +68:35:10.2
17:59:42.75 +68:20:14.0
18:00:25.60 +68:24:08.1
18:10:50.63 +68:41:09.8
18:27:43.07 +69:02:50.6
18:24:56.54 +69:03:40.3
18:26:20.10 +69:11:57.3
18:24:53.86 +69:15:06.5
18:24:28.37 +69:18:14.8
18:24:20.36 +69:18:31.7
19:00:00.02 +74:09:19.1
18:52:55.45 +73:42:20.2
########### Completed Dra-05-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 ####
19:01:00.92 +73:28:07.7
18:17:00.69 +67:59:47.9
18:00:52.12 +68:14:54.3
19:00:00.02 +74:09:19.1
18:19:31.62 +68:26:59.0
19:59:06.43 +68:18:48.1
19:59:35.99 +68:10:58.1
19:59:47.45 +68:17:17.7
19:54:13.35 +67:02:01.5
19:58:21.62 +68:22:24.6
18:00:25.60 +68:24:08.1
18:13:41.92 +68:35:10.2
18:24:56.54 +69:03:40.3
18:10:50.63 +68:41:09.8
18:11:38.58 +68:15:18.5
18:12:20.11 +68:04:42.3
18:27:43.07 +69:02:50.6
19:59:33.91 +68:13:06.5
18:24:53.86 +69:15:06.5
18:29:14.29 +67:46:23.9
18:33:01.55 +68:01:26.4
18:26:20.10 +69:11:57.3
19:59:21.79 +68:23:25.5
19:11:30.81 +68:14:09.5
18:29:25.77 +67:50:40.4
18:27:08.04 +67:57:25.4
19:59:46.61 +68:20:33.8
19:12:57.09 +68:10:42.4
18:20:32.17 +68:10:13.2
18:25:22.98 +68:01:13.2
17:59:42.75 +68:20:14.0
19:52:56.95 +67:35:21.9
18:15:47.95 +68:37:03.5
18:24:20.36 +69:18:31.7
18:24:28.37 +69:18:14.8
18:29:05.60 +67:42:17.8
18:52:55.45 +73:42:20.2
18:21:40.56 +68:15:50.6
###################################################################################
19:01:00.92 +73:28:07.7 -- not an asteroid (will add it to exclusion list)
18:17:00.69 +67:59:47.9 -- not an asteroid (will add it to exclusion list)
18:00:52.12 +68:14:54.3 -- not an asteroid (will add it to exclusion list)
19:00:00.02 +74:09:19.1 -- not an asteroid (will add it to exclusion list)
18:19:31.62 +68:26:59.0 -- not an asteroid (will add it to exclusion list)
19:59:06.43 +68:18:48.1 -- not an asteroid (will add it to exclusion list)
19:59:35.99 +68:10:58.1 -- not an asteroid (will add it to exclusion list)
19:59:47.45 +68:17:17.7 -- not an asteroid (will add it to exclusion list)
19:54:13.35 +67:02:01.5 -- not an asteroid (will add it to exclusion list)
19:58:21.62 +68:22:24.6 -- not an asteroid (will add it to exclusion list)
18:00:25.60 +68:24:08.1 -- not an asteroid (will add it to exclusion list)
18:13:41.92 +68:35:10.2 -- not an asteroid (will add it to exclusion list)
18:24:56.54 +69:03:40.3 -- not an asteroid (will add it to exclusion list)
18:10:50.63 +68:41:09.8 -- not an asteroid (will add it to exclusion list)
18:11:38.58 +68:15:18.5 -- not an asteroid (will add it to exclusion list)
18:12:20.11 +68:04:42.3 -- not an asteroid (will add it to exclusion list)
18:27:43.07 +69:02:50.6 -- not an asteroid (will add it to exclusion list)
19:59:33.91 +68:13:06.5 -- not an asteroid (will add it to exclusion list)
18:24:53.86 +69:15:06.5 -- not an asteroid (will add it to exclusion list)
18:29:14.29 +67:46:23.9 -- not an asteroid (will add it to exclusion list)
18:33:01.55 +68:01:26.4 -- not an asteroid (will add it to exclusion list)
18:26:20.10 +69:11:57.3 -- not an asteroid (will add it to exclusion list)
19:59:21.79 +68:23:25.5 -- not an asteroid (will add it to exclusion list)
19:11:30.81 +68:14:09.5 -- not an asteroid (will add it to exclusion list)
18:29:25.77 +67:50:40.4 -- not an asteroid (will add it to exclusion list)
18:27:08.04 +67:57:25.4 -- not an asteroid (will add it to exclusion list)
19:59:46.61 +68:20:33.8 -- not an asteroid (will add it to exclusion list)
19:12:57.09 +68:10:42.4 -- not an asteroid (will add it to exclusion list)
18:20:32.17 +68:10:13.2 -- not an asteroid (will add it to exclusion list)
18:25:22.98 +68:01:13.2 -- not an asteroid (will add it to exclusion list)
17:59:42.75 +68:20:14.0 -- not an asteroid (will add it to exclusion list)
19:52:56.95 +67:35:21.9 -- not an asteroid (will add it to exclusion list)
18:15:47.95 +68:37:03.5 -- not an asteroid (will add it to exclusion list)
18:24:20.36 +69:18:31.7 -- not an asteroid (will add it to exclusion list)
18:24:28.37 +69:18:14.8 -- not an asteroid (will add it to exclusion list)
18:29:05.60 +67:42:17.8 -- not an asteroid (will add it to exclusion list)
18:52:55.45 +73:42:20.2 -- not an asteroid (will add it to exclusion list)
18:21:40.56 +68:15:50.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:59:42.75 +68:20:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:00:25.60 +68:24:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:00:52.12 +68:14:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:50.63 +68:41:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:38.58 +68:15:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:20.11 +68:04:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:41.92 +68:35:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:47.95 +68:37:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:00.69 +67:59:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:19:31.62 +68:26:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:20:32.17 +68:10:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:21:40.56 +68:15:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:20.36 +69:18:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:28.37 +69:18:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:53.86 +69:15:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:24:56.54 +69:03:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:25:22.98 +68:01:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:20.10 +69:11:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:08.04 +67:57:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:43.07 +69:02:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:29:05.60 +67:42:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:29:14.29 +67:46:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:29:25.77 +67:50:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:33:01.55 +68:01:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:55.45 +73:42:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:00.02 +74:09:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:00.92 +73:28:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:30.81 +68:14:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:57.09 +68:10:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:56.95 +67:35:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:13.35 +67:02:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:21.62 +68:22:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:06.43 +68:18:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:21.79 +68:23:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:33.91 +68:13:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:35.99 +68:10:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:46.61 +68:20:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:47.45 +68:17:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
17:59:42.75 +68:20:14.0 -- not a known variable star
18:00:25.60 +68:24:08.1 -- not a known variable star
18:00:52.12 +68:14:54.3 -- not a known variable star
18:10:50.63 +68:41:09.8 -- not a known variable star
18:11:38.58 +68:15:18.5 -- not a known variable star
18:12:20.11 +68:04:42.3 -- not a known variable star
18:13:41.92 +68:35:10.2 -- not a known variable star
18:15:47.95 +68:37:03.5 -- not a known variable star
18:17:00.69 +67:59:47.9 -- not a known variable star
18:19:31.62 +68:26:59.0 -- not a known variable star
18:20:32.17 +68:10:13.2 -- not a known variable star
18:21:40.56 +68:15:50.6 -- not a known variable star
18:24:20.36 +69:18:31.7 -- not a known variable star
18:24:28.37 +69:18:14.8 -- not a known variable star
18:24:53.86 +69:15:06.5 -- not a known variable star
18:24:56.54 +69:03:40.3 -- not a known variable star
18:25:22.98 +68:01:13.2 -- not a known variable star
18:26:20.10 +69:11:57.3 -- not a known variable star
18:27:08.04 +67:57:25.4 -- not a known variable star
18:27:43.07 +69:02:50.6 -- not a known variable star
18:29:05.60 +67:42:17.8 -- not a known variable star
18:29:14.29 +67:46:23.9 -- not a known variable star
18:29:25.77 +67:50:40.4 -- a known variable star
18:33:01.55 +68:01:26.4 -- not a known variable star
18:52:55.45 +73:42:20.2 -- a known variable star
19:00:00.02 +74:09:19.1 -- not a known variable star
19:01:00.92 +73:28:07.7 -- not a known variable star
19:11:30.81 +68:14:09.5 -- not a known variable star
19:12:57.09 +68:10:42.4 -- not a known variable star
19:52:56.95 +67:35:21.9 -- a known variable star
19:54:13.35 +67:02:01.5 -- not a known variable star
19:58:21.62 +68:22:24.6 -- not a known variable star
19:59:06.43 +68:18:48.1 -- not a known variable star
19:59:21.79 +68:23:25.5 -- not a known variable star
19:59:33.91 +68:13:06.5 -- not a known variable star
19:59:35.99 +68:10:58.1 -- not a known variable star
19:59:46.61 +68:20:33.8 -- not a known variable star
19:59:47.45 +68:17:17.7 -- not a known variable star
Found 35 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:59:42.75 +68:20:14.0
18:00:25.60 +68:24:08.1
18:00:52.12 +68:14:54.3
18:10:50.63 +68:41:09.8
18:11:38.58 +68:15:18.5
18:12:20.11 +68:04:42.3
18:13:41.92 +68:35:10.2
18:15:47.95 +68:37:03.5
18:17:00.69 +67:59:47.9
18:19:31.62 +68:26:59.0
18:20:32.17 +68:10:13.2
18:21:40.56 +68:15:50.6
18:24:20.36 +69:18:31.7
18:24:28.37 +69:18:14.8
18:24:53.86 +69:15:06.5
18:24:56.54 +69:03:40.3
18:25:22.98 +68:01:13.2
18:26:20.10 +69:11:57.3
18:27:08.04 +67:57:25.4
18:27:43.07 +69:02:50.6
18:29:05.60 +67:42:17.8
18:29:14.29 +67:46:23.9
18:29:25.77 +67:50:40.4
18:33:01.55 +68:01:26.4
18:52:55.45 +73:42:20.2
19:00:00.02 +74:09:19.1
19:01:00.92 +73:28:07.7
19:11:30.81 +68:14:09.5
19:12:57.09 +68:10:42.4
19:52:56.95 +67:35:21.9
19:54:13.35 +67:02:01.5
19:58:21.62 +68:22:24.6
19:59:06.43 +68:18:48.1
19:59:21.79 +68:23:25.5
19:59:33.91 +68:13:06.5
19:59:35.99 +68:10:58.1
19:59:46.61 +68:20:33.8
19:59:47.45 +68:17:17.7
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461239.76061087 -observatory V36
07:12:34.83 +17:30:53.7 Mercury (4.0mag)
10:44:02.77 +09:05:50.7 Venus (-4.2mag)
04:47:37.09 +22:18:16.4 Mars (1.3mag)
08:23:52.83 +19:48:13.5 Jupiter (-1.8mag)
00:56:31.56 +03:22:19.7 Saturn (0.7mag)
04:08:40.82 +20:48:56.2 Uranus (5.8mag)
00:16:55.65 +00:19:36.4 Neptune (7.7mag)
20:30:10.39 -23:21:29.1 Pluto (14.4mag)
11:06:54.65 +03:10:28.4 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 04:27 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.76061087:
08:23:49.84 +19:48:24.8 Io (6.0mag)
08:24:04.21 +19:47:29.9 Europa (6.3mag)
08:24:09.12 +19:47:09.4 Ganymede (5.6mag)
08:23:26.75 +19:49:54.5 Callisto (6.8mag)
08:22:03.65 +19:35:56.4 Himalia (15.7mag)
08:23:52.05 +19:48:17.6 Thebe (16.6mag)
08:21:24.67 +19:38:40.5 Elara (17.7mag)
08:27:38.62 +19:38:11.3 Pasiphae (17.9mag)
08:28:23.05 +19:54:30.5 Carme (19.0mag)
00:56:41.85 +03:22:27.0 Titan (8.5mag)
00:56:31.32 +03:22:29.8 Rhea (9.8mag)
00:55:57.06 +03:20:10.2 Iapetus (11.2mag)
00:56:18.42 +03:22:10.8 Hyperion (14.5mag)
00:56:21.71 +03:18:24.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 04:27 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.76061087:
17:58:54.46 -31:05:29.3 JWST
16:12:18.56 +49:58:17.1 Chandra
22:06:53.41 +54:43:52.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 04:27 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.76061087 -observatory V36
02:47:18.87 +15:20:20.7 17.8mag P/1996 R2 (Lagerkvist)
18:12:09.71 -34:32:35.2 13.8mag P/2010 H2 (Vales)
06:33:33.72 -68:17:05.9 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:30.27 +32:35:04.9 17.6mag C/2017 K2 (PANSTARRS)
02:28:07.81 +21:14:29.2 15.8mag P/2021 N1 (ZTF)
22:54:31.23 +32:13:29.9 17.3mag C/2022 E2 (ATLAS)
06:21:19.50 +26:50:49.4 16.7mag C/2022 N2 (PANSTARRS)
10:02:28.52 +29:25:28.1 16.9mag C/2022 QE78 (ATLAS)
09:14:53.02 +05:07:58.8 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.75 -11:35:05.5 17.8mag P/2023 B1 (PANSTARRS)
21:39:17.18 +67:29:04.8 17.9mag C/2023 H5 (Lemmon)
16:16:12.40 -10:53:44.9 14.0mag C/2023 R1 (PANSTARRS)
08:14:36.27 +66:08:55.4 17.9mag C/2024 A1 (ATLAS)
07:43:01.44 +30:23:38.7 14.8mag C/2024 E1 (Wierzchos)
15:12:48.48 +15:30:01.4 17.6mag C/2024 G6 (ATLAS)
19:31:00.37 +40:48:49.5 13.7mag C/2024 J3 (ATLAS)
21:38:53.78 +47:07:52.7 17.8mag C/2024 R4 (PANSTARRS)
04:57:00.98 -13:28:09.3 15.7mag C/2024 T5 (ATLAS)
06:41:00.24 +27:44:52.0 18.0mag C/2025 J1 (Borisov)
07:19:39.18 -13:38:03.0 16.9mag C/2025 R3 (PANSTARRS)
10:05:29.21 +22:04:41.9 17.5mag C/2025 V2 (Rankin)
12:47:31.39 +03:34:30.4 17.0mag C/2025 Y1 (ATLAS)
16:31:04.61 +79:07:46.4 17.2mag C/2026 A2 (Bok)
02:54:06.19 +45:33:54.0 16.8mag C/2026 B2 (Sun-Gao)
11:30:45.70 +05:51:50.2 17.0mag A/2026 E1
21:31:08.29 -18:06:45.1 7.1mag 10P/Tempel
11:17:18.24 -02:14:39.3 16.2mag 29P/Schwassmann-Wachmann
04:11:26.72 +30:23:49.0 17.9mag 47P/Ashbrook-Jackson
10:24:33.62 +11:28:34.0 17.1mag 63P/Wild
00:51:23.38 -05:02:47.8 15.5mag 65P/Gunn
04:46:27.60 +20:31:34.0 13.7mag 78P/Gehrels
02:34:39.54 +11:38:38.2 16.4mag 88P/Howell
06:58:46.25 +29:59:02.3 15.8mag 93P/Lovas
04:46:52.16 +31:19:48.6 16.7mag 114P/Wiseman-Skiff
08:28:00.50 +29:46:03.5 15.2mag 123P/West-Hartley
11:02:59.29 -02:00:56.5 16.9mag 124P/Mrkos
05:04:22.02 +21:00:36.5 16.2mag 128P/Shoemaker-Holt
05:51:03.96 +19:36:48.4 17.8mag 131P/Mueller
07:41:42.12 +15:15:35.9 16.5mag 141P-D/Machholz
03:20:17.92 -20:45:05.5 15.1mag 161P/Hartley-IRAS
06:01:36.40 +35:29:42.4 15.5mag 162P/SidingSpring
18:39:21.05 +20:30:18.8 14.0mag 169P/NEAT
01:59:33.50 +08:24:24.5 17.6mag 220P/McNaught
16:35:32.55 -08:44:35.9 17.2mag 235P/LINEAR
09:01:49.46 +32:32:33.4 18.0mag 240P/NEAT
20:37:57.45 -51:08:32.4 17.8mag 259P/Garradd
02:21:35.58 +15:47:15.6 15.6mag 260P/McNaught
06:01:19.74 +37:23:08.6 17.3mag 295P/LINEAR
15:06:33.42 +05:19:32.9 17.6mag 391P/Kowalski
08:41:44.60 +19:20:48.3 17.9mag 450P/LONEOS
08:04:06.91 +38:33:10.5 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 04:27 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 18 04:27 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 18 04:27 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
21:57:43.950 -02:48:28.98 AT 2026svg 2026-06-26.41 21.5213
-rw-r--r-- 1 apache apache 89K Jul 18 04:27 tns_transients_list.txt
