This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.51 11:30:29.02 +66:13:59.6
135.18223 48.92473 galactic Dra Second-epoch detections are separated by 2.5" and 7.7 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 | 11:30:29.02 +66:13:59.6 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:29.02 +66:13:59.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:29.02 +66:13:59.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461258.7362,12.51,0.05,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 20260806.2362 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.41 11:21:40.59 +66:34:29.0
136.09118 48.19575 galactic UMa Second-epoch detections are separated by 1.6" and 7.7 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 | 11:21:40.59 +66:34:29.0 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:40.59 +66:34:29.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:40.59 +66:34:29.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 21 40.59 +66 34 29.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.41,0.05,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 20260806.2362 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 08 06.2362 2461258.7362 12.43 11:30:29.02 +65:52:09.0
135.44353 49.24605 galactic Dra Second-epoch detections are separated by 1.7" and 7.7 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 | 11:30:29.02 +65:52:09.0 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:29.02 +65:52:09.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:29.02 +65:52:09.0: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.67 11:20:17.07 +65:56:09.8
136.76864 48.67061 galactic UMa Second-epoch detections are separated by 2.2" and 7.4 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 | 11:20:17.07 +65:56:09.8 (user input) | T | P | (position from user input) J-Ks=0.720+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:17.07 +65:56:09.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:17.07 +65:56:09.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 20 17.07 +65 56 09.8 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.47 11:15:59.76 +66:32:23.4
136.83875 47.92969 galactic UMa Second-epoch detections are separated by 1.2" and 7.8 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 | 11:15:59.76 +66:32:23.4 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:59.76 +66:32:23.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:59.76 +66:32:23.4: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 15 59.76 +66 32 23.4 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.80 12:50:16.57 +70:34:01.0
123.07245 46.56099 galactic Dra Second-epoch detections are separated by 2.4" and 7.1 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 | 12:50:16.57 +70:34:01.0 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.035 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:50:16.57 +70:34:01.0: 13.79 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:50:16.57 +70:34:01.0: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461258.7362,12.80,0.05,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 20260806.2362 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 08 06.2362 2461258.7362 12.64 11:24:32.01 +66:33:05.8
135.73965 48.35855 galactic UMa Second-epoch detections are separated by 2.4" and 7.9 pix
The object was not found in VSX
The object was found in ASASSN-V13" ASASSN-V J112434.10+663303.5
Type: VAR
MeanMag 13.97 m Amp. 0.09 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:32.01 +66:33:05.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:24:32.01 +66:33:05.8: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 24 32.01 +66 33 05.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.7362,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.2362 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.56 11:18:08.11 +66:41:43.2
136.44716 47.91079 galactic UMa Second-epoch detections are separated by 1.8" and 7.8 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 | Large-amplitude variable Gaia DR2 1060607131109853952 | 11:18:08.11 +66:41:43.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.800+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:08.11 +66:41:43.2: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:08.11 +66:41:43.2: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 08.11 +66 41 43.2 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1060607131109853952,2461258.7362,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1060607131109853952 20260806.2362 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.43 11:22:20.00 +66:20:35.7
136.18346 48.42837 galactic UMa Second-epoch detections are separated by 1.4" and 7.5 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 | 11:22:20.00 +66:20:35.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:20.00 +66:20:35.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:20.00 +66:20:35.7: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 22 20.00 +66 20 35.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.57 11:28:31.87 +65:34:40.9
135.92748 49.40590 galactic UMa Second-epoch detections are separated by 1.5" and 7.5 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 | 11:28:31.87 +65:34:40.9 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:31.87 +65:34:40.9: 13.63 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:31.87 +65:34:40.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 28 31.87 +65 34 40.9 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.58 11:19:53.39 +65:59:49.1
136.77230 48.59767 galactic UMa Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:19:53.39 +65:59:49.1 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:53.39 +65:59:49.1: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:53.39 +65:59:49.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 19 53.39 +65 59 49.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.47 11:25:36.79 +65:39:24.2
136.27049 49.18945 galactic UMa Second-epoch detections are separated by 1.3" and 7.7 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 | 11:25:36.79 +65:39:24.2 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:36.79 +65:39:24.2: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:25:36.79 +65:39:24.2: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 25 36.79 +65 39 24.2 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.64 11:17:41.99 +66:51:27.0
136.37444 47.75030 galactic UMa Second-epoch detections are separated by 3.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:17:41.99 +66:51:27.0 (user input) | T | P | (position from user input) J-Ks=0.770+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:41.99 +66:51:27.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:41.99 +66:51:27.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 41.99 +66 51 27.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.48 11:26:49.56 +65:51:43.6
135.94998 49.07241 galactic UMa Second-epoch detections are separated by 2.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:26:49.56 +65:51:43.6 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:49.56 +65:51:43.6: 13.59 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:49.56 +65:51:43.6: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 26 49.56 +65 51 43.6 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.51 11:17:49.52 +65:43:08.0
137.26635 48.72175 galactic UMa Second-epoch detections are separated by 0.5" and 7.7 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 | 11:17:49.52 +65:43:08.0 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:49.52 +65:43:08.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:49.52 +65:43:08.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 49.52 +65 43 08.0 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.51,0.05,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 20260806.2362 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.55 11:31:37.02 +65:50:24.0
135.30755 49.32615 galactic Dra Second-epoch detections are separated by 1.7" and 7.8 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 | 11:31:37.02 +65:50:24.0 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.033 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:31:37.02 +65:50:24.0: 13.55 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:31:37.02 +65:50:24.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461258.7362,12.55,0.05,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 20260806.2362 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.41 11:23:42.15 +65:54:29.5
136.33654 48.87361 galactic UMa Second-epoch detections are separated by 1.9" and 7.3 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 | 11:23:42.15 +65:54:29.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:42.15 +65:54:29.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:42.15 +65:54:29.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 23 42.15 +65 54 29.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.41,0.05,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 20260806.2362 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 08 06.2362 2461258.7362 12.58 11:15:47.56 +66:58:04.9
136.52268 47.55742 galactic UMa Second-epoch detections are separated by 2.4" and 7.7 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 | 11:15:47.56 +66:58:04.9 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.034 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:47.56 +66:58:04.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:47.56 +66:58:04.9: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 15 47.56 +66 58 04.9 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.48 11:17:42.71 +66:24:33.4
136.72644 48.13148 galactic UMa Second-epoch detections are separated by 4.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:17:42.71 +66:24:33.4 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:42.71 +66:24:33.4: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:42.71 +66:24:33.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 42.71 +66 24 33.4 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.41 11:18:49.50 +66:25:58.1
136.56609 48.17021 galactic UMa Second-epoch detections are separated by 1.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:49.50 +66:25:58.1 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.056 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:49.50 +66:25:58.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:49.50 +66:25:58.1: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 49.50 +66 25 58.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.41,0.05,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 20260806.2362 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 08 06.2362 2461258.7362 12.46 11:30:22.96 +65:45:37.9
135.53619 49.33692 galactic UMa Second-epoch detections are separated by 2.5" and 7.8 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 | 11:30:22.96 +65:45:37.9 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.033 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:22.96 +65:45:37.9: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:22.96 +65:45:37.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 30 22.96 +65 45 37.9 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.40 11:18:34.24 +65:21:00.1
137.46781 49.07456 galactic UMa Second-epoch detections are separated by 2.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:34.24 +65:21:00.1 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:34.24 +65:21:00.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:34.24 +65:21:00.1: 13.47 +/- 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!
TCP 2026 08 06.2362* 11 18 34.24 +65 21 00.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.40,0.05,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 20260806.2362 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.50 11:18:54.09 +66:43:05.9
136.33291 47.93090 galactic UMa Second-epoch detections are separated by 4.1" and 7.7 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 | 11:18:54.09 +66:43:05.9 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:54.09 +66:43:05.9: 13.45 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:54.09 +66:43:05.9: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 54.09 +66 43 05.9 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.50,0.05,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 20260806.2362 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.43 11:35:09.59 +65:38:46.2
134.94602 49.66502 galactic UMa Second-epoch detections are separated by 1.3" and 7.7 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 | 11:35:09.59 +65:38:46.2 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:09.59 +65:38:46.2: 13.39 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:35:09.59 +65:38:46.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 35 09.59 +65 38 46.2 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.38 11:19:44.76 +65:34:05.5
137.13334 48.95469 galactic UMa Second-epoch detections are separated by 1.8" and 7.4 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 | 11:19:44.76 +65:34:05.5 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:44.76 +65:34:05.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:44.76 +65:34:05.5: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 19 44.76 +65 34 05.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.27 11:28:36.37 +65:30:48.6
135.96507 49.46612 galactic UMa Second-epoch detections are separated by 1.6" and 7.7 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 | 11:28:36.37 +65:30:48.6 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.025 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:36.37 +65:30:48.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:36.37 +65:30:48.6: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 28 36.37 +65 30 48.6 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.39 11:16:51.85 +66:18:19.8
136.91712 48.17403 galactic UMa Second-epoch detections are separated by 2.3" and 7.7 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 | 11:16:51.85 +66:18:19.8 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:51.85 +66:18:19.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:51.85 +66:18:19.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 16 51.85 +66 18 19.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.32 11:21:21.58 +66:23:43.7
136.26963 48.33365 galactic UMa Second-epoch detections are separated by 1.1" and 7.7 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 | 11:21:21.58 +66:23:43.7 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:21.58 +66:23:43.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:21.58 +66:23:43.7: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 21 21.58 +66 23 43.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.32 11:30:39.29 +66:03:20.7
135.28578 49.08960 galactic Dra Second-epoch detections are separated by 0.6" and 7.8 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 | 11:30:39.29 +66:03:20.7 (user input) | T | P | (position from user input) J-Ks=0.546+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:39.29 +66:03:20.7: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:39.29 +66:03:20.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.29 11:17:24.08 +66:46:38.2
136.47455 47.80296 galactic UMa Second-epoch detections are separated by 0.6" and 7.5 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 | 11:17:24.08 +66:46:38.2 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:24.08 +66:46:38.2: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:24.08 +66:46:38.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 24.08 +66 46 38.2 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.31 11:20:46.39 +66:21:11.4
136.37817 48.33971 galactic UMa Second-epoch detections are separated by 1.6" and 7.9 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 | 11:20:46.39 +66:21:11.4 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:46.39 +66:21:11.4: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:46.39 +66:21:11.4: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 20 46.39 +66 21 11.4 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.23 11:16:37.39 +66:27:07.6
136.83016 48.03726 galactic UMa Second-epoch detections are separated by 0.9" and 7.5 pix
The object was found in VSX 2" Gaia DR3 1057593129220029824
Type: ROT
# Max. Min./Amp. JD0 Period
13.000 G 13.030 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:37.39 +66:27:07.6: 13.28 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:37.39 +66:27:07.6: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 16 37.39 +66 27 07.6 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057593129220029824,2461258.7362,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057593129220029824 20260806.2362 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.39 11:15:38.89 +66:35:17.0
136.84354 47.87043 galactic UMa Second-epoch detections are separated by 1.0" and 7.8 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 | 11:15:38.89 +66:35:17.0 (user input) | T | P | (position from user input) J-Ks=0.605+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:38.89 +66:35:17.0: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:38.89 +66:35:17.0: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 15 38.89 +66 35 17.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.25 11:18:33.65 +66:38:58.6
136.42944 47.97182 galactic UMa Second-epoch detections are separated by 2.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:33.65 +66:38:58.6 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.027 (M)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:33.65 +66:38:58.6: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:33.65 +66:38:58.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 33.65 +66 38 58.6 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.28 11:29:00.93 +65:42:14.7
135.76695 49.31956 galactic UMa Second-epoch detections are separated by 2.5" and 7.2 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 | 11:29:00.93 +65:42:14.7 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.032 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:00.93 +65:42:14.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:00.93 +65:42:14.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 29 00.93 +65 42 14.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.25 11:20:53.91 +65:29:51.3
137.03509 49.07746 galactic UMa Second-epoch detections are separated by 1.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:20:53.91 +65:29:51.3 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:53.91 +65:29:51.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:53.91 +65:29:51.3: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 20 53.91 +65 29 51.3 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.15 11:21:51.58 +66:21:19.7
136.23566 48.39365 galactic UMa Second-epoch detections are separated by 1.5" and 7.7 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 | 11:21:51.58 +66:21:19.7 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:51.58 +66:21:19.7: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:51.58 +66:21:19.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 21 51.58 +66 21 19.7 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.23 11:16:10.50 +66:30:57.9
136.83534 47.95929 galactic UMa Second-epoch detections are separated by 2.3" and 7.3 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 | 11:16:10.50 +66:30:57.9 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:10.50 +66:30:57.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:10.50 +66:30:57.9: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 16 10.50 +66 30 57.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.16 11:22:21.24 +65:45:24.9
136.63446 48.93347 galactic UMa Second-epoch detections are separated by 1.0" and 7.7 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 | 11:22:21.24 +65:45:24.9 (user input) | T | P | (position from user input) J-Ks=0.647+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:21.24 +65:45:24.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:21.24 +65:45:24.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 22 21.24 +65 45 24.9 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.15 11:17:03.09 +66:06:59.0
137.04530 48.34385 galactic UMa Second-epoch detections are separated by 1.4" and 7.8 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 | 11:17:03.09 +66:06:59.0 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:03.09 +66:06:59.0: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:03.09 +66:06:59.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 03.09 +66 06 59.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.16 11:21:01.67 +66:00:04.4
136.61947 48.65429 galactic UMa Second-epoch detections are separated by 0.7" and 7.5 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 | 11:21:01.67 +66:00:04.4 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:01.67 +66:00:04.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:01.67 +66:00:04.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 21 01.67 +66 00 04.4 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.11 11:20:40.96 +66:31:47.4
136.25303 48.18366 galactic UMa Second-epoch detections are separated by 1.5" and 7.7 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 | 11:20:40.96 +66:31:47.4 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.031 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:40.96 +66:31:47.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:40.96 +66:31:47.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 20 40.96 +66 31 47.4 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.18 11:33:00.60 +65:49:28.0
135.12449 49.40588 galactic Dra Second-epoch detections are separated by 1.7" and 7.3 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 | 11:33:00.60 +65:49:28.0 (user input) | T | P | (position from user input) J-Ks=0.285+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:33:00.60 +65:49:28.0: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:33:00.60 +65:49:28.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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,2461258.7362,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.95 11:30:06.93 +65:40:05.5
135.64056 49.40519 galactic UMa Second-epoch detections are separated by 0.7" and 7.7 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 | 11:30:06.93 +65:40:05.5 (user input) | T | P | (position from user input) J-Ks=0.516+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:06.93 +65:40:05.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:06.93 +65:40:05.5: 12.97 +/- 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!
TCP 2026 08 06.2362* 11 30 06.93 +65 40 05.5 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.99 11:22:00.07 +65:49:06.7
136.63349 48.86203 galactic UMa Second-epoch detections are separated by 2.4" and 7.5 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 | 11:22:00.07 +65:49:06.7 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:00.07 +65:49:06.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:00.07 +65:49:06.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 22 00.07 +65 49 06.7 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.97 11:22:15.25 +66:10:00.8
136.32940 48.57608 galactic UMa Second-epoch detections are separated by 0.4" and 7.7 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 | 11:22:15.25 +66:10:00.8 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:15.25 +66:10:00.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:15.25 +66:10:00.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 22 15.25 +66 10 00.8 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 12.01 11:29:29.34 +65:31:23.7
135.83449 49.50166 galactic UMa Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:29:29.34 +65:31:23.7 (user input) | T | P | (position from user input) J-Ks=0.251+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:29.34 +65:31:23.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:29.34 +65:31:23.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 29 29.34 +65 31 23.7 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,12.01,0.05,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 20260806.2362 12.01CV 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 08 06.2362 2461258.7362 11.96 11:22:07.88 +65:56:21.0
136.52204 48.76536 galactic UMa Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:22:07.88 +65:56:21.0 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:07.88 +65:56:21.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:07.88 +65:56:21.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 22 07.88 +65 56 21.0 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.96,0.05,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 20260806.2362 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.71 11:19:08.07 +65:21:59.9
137.37840 49.09191 galactic UMa Second-epoch detections are separated by 0.5" and 7.8 pix
The object was found in VSX21" Gaia DR3 1057241800895191040
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.720 G G
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:08.07 +65:21:59.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:08.07 +65:21:59.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 19 08.07 +65 21 59.9 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057241800895191040,2461258.7362,11.71,0.05,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
Gaia DR3 1057241800895191040 20260806.2362 11.71CV 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 08 06.2362 2461258.7362 11.84 11:24:26.74 +65:41:49.9
136.39856 49.09421 galactic UMa Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1057275713956883072
Type: ROT
# Max. Min./Amp. JD0 Period
12.600 G 12.650 G G
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:26.74 +65:41:49.9: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:24:26.74 +65:41:49.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 24 26.74 +65 41 49.9 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057275713956883072,2461258.7362,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057275713956883072 20260806.2362 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.84 11:31:12.33 +65:49:20.5
135.37733 49.32207 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:31:12.33 +65:49:20.5 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:31:12.33 +65:49:20.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:31:12.33 +65:49:20.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.81 11:32:42.51 +65:48:12.9
135.18138 49.41021 galactic UMa Second-epoch detections are separated by 1.1" and 7.7 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 | 11:32:42.51 +65:48:12.9 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:32:42.51 +65:48:12.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:32:42.51 +65:48:12.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 32 42.51 +65 48 12.9 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.2362 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.71 11:21:05.17 +65:38:58.2
136.88900 48.95799 galactic UMa Second-epoch detections are separated by 0.6" and 7.7 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 | 11:21:05.17 +65:38:58.2 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:05.17 +65:38:58.2: 12.72 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:05.17 +65:38:58.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 21 05.17 +65 38 58.2 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.71,0.05,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 20260806.2362 11.71CV 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 08 06.2362 2461258.7362 11.71 11:16:45.89 +66:12:47.6
137.00399 48.24658 galactic UMa Second-epoch detections are separated by 0.5" and 7.7 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 | 11:16:45.89 +66:12:47.6 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:45.89 +66:12:47.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:45.89 +66:12:47.6: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 16 45.89 +66 12 47.6 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.7362,11.71,0.05,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 20260806.2362 11.71CV 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 08 06.2362 2461258.7362 11.67 11:18:55.72 +66:13:12.6
136.72060 48.35661 galactic UMa Second-epoch detections are separated by 1.2" and 7.5 pix
The object was found in VSX 1" Gaia DR3 1057532827879179648
Type: ROT
# Max. Min./Amp. JD0 Period
12.470 G 12.490 G G
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:55.72 +66:13:12.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:55.72 +66:13:12.6: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 55.72 +66 13 12.6 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057532827879179648,2461258.7362,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057532827879179648 20260806.2362 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.71 11:27:23.60 +65:47:45.3
135.92205 49.15856 galactic UMa Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057362231778221824 | 11:27:23.67 +65:47:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.488+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:27:23.60 +65:47:45.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:27:23.60 +65:47:45.3: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 27 23.60 +65 47 45.3 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057362231778221824,2461258.7362,11.71,0.05,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
Gaia DR3 1057362231778221824 20260806.2362 11.71CV 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 08 06.2362 2461258.7362 11.47 11:17:45.49 +65:49:44.3
137.18589 48.62509 galactic UMa Second-epoch detections are separated by 1.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1057503793900278400 | 11:17:45.59 +65:49:44.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.493+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:45.49 +65:49:44.3: 12.43 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:45.49 +65:49:44.3: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 45.49 +65 49 44.3 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1057503793900278400,2461258.7362,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1057503793900278400 20260806.2362 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.39 11:17:20.68 +65:59:01.1
137.11462 48.47187 galactic UMa Second-epoch detections are separated by 0.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057509531977038464 | 11:17:20.63 +65:59:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.706+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:20.68 +65:59:01.1: 12.34 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:20.68 +65:59:01.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 17 20.68 +65 59 01.1 11.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057509531977038464,2461258.7362,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057509531977038464 20260806.2362 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 11.28 11:18:57.79 +65:48:31.8
137.04396 48.70783 galactic UMa Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057321240610283904 | 11:18:57.77 +65:48:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.743+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:57.79 +65:48:31.8: 12.28 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:57.79 +65:48:31.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 18 57.79 +65 48 31.8 11.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057321240610283904,2461258.7362,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057321240610283904 20260806.2362 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2362 2461258.7362 10.96 11:26:28.05 +65:36:26.1
136.19092 49.27613 galactic UMa Second-epoch detections are separated by 1.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1056515431730737280 | 11:26:28.15 +65:36:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.529+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:28.05 +65:36:26.1: 11.93 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:28.05 +65:36:26.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2362* 11 26 28.05 +65 36 26.1 11.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1056515431730737280,2461258.7362,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1056515431730737280 20260806.2362 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461258.73658852 06.08.2026 05:40:31.248 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6107
Objects passed selection criteria: 6069
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 3580
Average stars matched: 3316.75 (92.6466 %)
Memory usage VmPeak: 232700 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 00:45:36 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: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461258.73658852 06.08.2026 05:40:31.248 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 182
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 34787
Objects passed selection criteria: 34662
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 21350
Average stars matched: 19706.8 (92.3033 %)
Memory usage VmPeak: 257664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 00:46:14 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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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: 2461258.73588348
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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits'
wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits'
wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:37.825 +69:59:43.99 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Image size: 937.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:04.084 +70:03:47.06 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 12:00:04.084 +70:03:47.06
Angular distance between the image centers 0.0772 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Image size: 937.7'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:59:58.835 +70:04:19.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 11:59:58.835 +70:04:19.57
Angular distance between the image centers 0.0822 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 12:00:04.084 +70:03:47.06
Second-epoch second image center 11:59:58.835 +70:04:19.57
Angular distance between the image centers 0.01171 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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.4gUJxRqYiK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits &> /tmp/tmp.OMR4KqPH5J
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits &> /tmp/tmp.OyPez15vWk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits &> /tmp/tmp.bpthfa3DrF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6391 to 206.7194 deg, Dec +62.8277 to +75.5472 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 151.6391 to 206.7194 deg, Dec 62.8277 to 75.5472 deg
Loaded 8255 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): 4552 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.845850
a=0.000000 b=1.000000 c=22.845850
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6391 to 206.7194 deg, Dec +62.8277 to +75.5472 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 151.6391 to 206.7194 deg, Dec 62.8277 to 75.5472 deg
Loaded 8255 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): 4552 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=6.1)
Read 8065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6392 to 206.7189 deg, Dec +62.8276 to +75.5471 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 151.6392 to 206.7189 deg, Dec 62.8276 to 75.5471 deg
Loaded 8255 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): 4558 out of 4791 total matches.
Matched with Tycho-2 4791 out of 8065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.2 pix Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
2.3 pix fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
2.4 pix fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Limiting magnitude estimates:
15.3 mag. Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.3 mag. Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
12.8 mag. fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
12.6 mag. fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4gUJxRqYiK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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=549, bad_region=1822, passed=7645
Got 7645 stars (including 5397 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 7645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=4901 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.343 n_q1=1490 n_q2=854 n_q3=1601 n_q4=956 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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.OMR4KqPH5J (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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=588, bad_region=1916, passed=8065
Got 8065 stars (including 5698 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 8065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 4899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 6575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 6575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 6575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4899 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits N_match=4899 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.400 sigma_q3_arcsec=0.355 sigma_q4_arcsec=0.373 n_q1=1497 n_q2=834 n_q3=1609 n_q4=959 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -region wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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.OyPez15vWk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=93, bad_region=428, passed=1641
Got 1641 stars (including 1140 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 1641 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 1108 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1106 matched stars entering correct_measured_positions(), 1090 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1106 matched stars entering correct_measured_positions(), 1240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 1109 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1105 matched stars entering correct_measured_positions(), 1241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 1105 matched stars entering correct_measured_positions(), 1241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 1105 stars left (next iteration limit 1216)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1105 robust_rms=7.104 arcsec worst_quadrant_rms=12.765 arcsec
SIP_REFIT: SIP order 3 trial: matched=1105 robust_rms=0.453 arcsec worst_quadrant_rms=0.497 arcsec
SIP_REFIT: SIP order 5 trial: matched=1105 robust_rms=0.352 arcsec worst_quadrant_rms=0.430 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1105 robust_rms_before=0.812 arcsec robust_rms_before_corrected=0.408 arcsec robust_rms_after=0.352 arcsec worst_quadrant_rms_before=0.473 worst_quadrant_rms_after=0.430
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.473 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits N_match=1105 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.477 n_q1=518 n_q2=110 n_q3=312 n_q4=165 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits -region wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.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.bpthfa3DrF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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=86, bad_region=466, passed=1673
Got 1673 stars (including 1139 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 1673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 769 to 828 (Dec 63.8 to 75.3)
Done reading UCAC5 zone files...
Matched 1108 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1106 matched stars entering correct_measured_positions(), 1092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1106 matched stars entering correct_measured_positions(), 1258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 769 to 828 (Dec 63.8 to 75.3)
Done reading UCAC5 zone files...
Matched 1108 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1104 matched stars entering correct_measured_positions(), 1258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 1104 matched stars entering correct_measured_positions(), 1257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 1104 stars left (next iteration limit 1216)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1104 robust_rms=7.067 arcsec worst_quadrant_rms=11.567 arcsec
SIP_REFIT: SIP order 3 trial: matched=1104 robust_rms=0.437 arcsec worst_quadrant_rms=0.496 arcsec
SIP_REFIT: SIP order 5 trial: matched=1104 robust_rms=0.356 arcsec worst_quadrant_rms=0.418 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1104 robust_rms_before=0.823 arcsec robust_rms_before_corrected=0.436 arcsec robust_rms_after=0.356 arcsec worst_quadrant_rms_before=0.474 worst_quadrant_rms_after=0.418
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Image size: 938.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:59:58.698 +70:04:19.43 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1673 stars ###
'wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/correct_sextractor_wcs_catalog_usingxy2sky915857.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.823 -> 0.356 arcsec)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits N_match=1104 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.393 n_q1=520 n_q2=115 n_q3=260 n_q4=209 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits -region wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits sigma_overall=0.368 worst_q_ratio=1.221
ref2=Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits sigma_overall=0.399 worst_q_ratio=1.154
new1=fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits sigma_overall=0.420 worst_q_ratio=1.135
new2=fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits sigma_overall=0.368 worst_q_ratio=1.134
reference average sigma_overall=0.3835 worst_q_ratio=1.1875
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294_astrometric_residuals.png (4901 matched stars from wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266_astrometric_residuals.png (4899 matched stars from wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212_astrometric_residuals.png (1105 matched stars from wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213_astrometric_residuals.png (1104 matched stars from wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits'
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-03-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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:37.825 +69:59:43.99 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Image size: 937.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:04.084 +70:03:47.06 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 12:00:04.084 +70:03:47.06
Angular distance between the image centers 0.0772 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Image size: 937.7'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:59:58.835 +70:04:19.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 11:59:58.835 +70:04:19.57
Angular distance between the image centers 0.0822 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 12:00:04.084 +70:03:47.06
Second-epoch second image center 11:59:58.835 +70:04:19.57
Angular distance between the image centers 0.01171 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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.kROpR8NHYF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits &> /tmp/tmp.cSZjxfLRoO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits &> /tmp/tmp.ARQZxrQZVD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits &> /tmp/tmp.wqPS7fyBWb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 to 206.9070 deg, Dec +62.7295 to +75.5590 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 151.3623 to 206.9070 deg, Dec 62.7295 to 75.5590 deg
Loaded 8398 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): 4346 out of 4840 total matches.
Matched with Tycho-2 4840 out of 42210 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.724350
a=0.000000 b=1.000000 c=22.724350
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 to 206.9070 deg, Dec +62.7295 to +75.5590 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 151.3623 to 206.9070 deg, Dec 62.7295 to 75.5590 deg
Loaded 8398 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): 4346 out of 4840 total matches.
Matched with Tycho-2 4840 out of 42210 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=4.7)
Read 42755 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3622 to 206.9063 deg, Dec +62.7295 to +75.5596 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 151.3622 to 206.9063 deg, Dec 62.7295 to 75.5596 deg
Loaded 8399 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): 4309 out of 4838 total matches.
Matched with Tycho-2 4838 out of 42755 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
2.2 pix fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
2.2 pix fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Limiting magnitude estimates:
15.5 mag. Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.5 mag. Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
13.2 mag. fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
13.1 mag. fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.7 (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.kROpR8NHYF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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=11, blended=2006, bad_region=8242, passed=42199
Got 42199 stars (including 32315 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 42199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=4907 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.324 n_q1=1489 n_q2=837 n_q3=1616 n_q4=965 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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.cSZjxfLRoO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2163, bad_region=8480, passed=42737
Got 42737 stars (including 32497 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 42737 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4897 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits N_match=4897 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.344 n_q1=1485 n_q2=827 n_q3=1620 n_q4=965 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -region wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.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.ARQZxrQZVD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.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=1, blended=342, bad_region=1806, passed=10734
Got 10734 stars (including 8728 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 10734 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 9313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 9313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 9313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits N_match=4864 sigma_overall_arcsec=0.531 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.523 sigma_q4_arcsec=0.570 n_q1=2326 n_q2=552 n_q3=1364 n_q4=622 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits -region wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.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.wqPS7fyBWb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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=338, bad_region=1958, passed=10706
Got 10706 stars (including 8550 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 10706 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 9187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 9187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4867 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits N_match=4867 sigma_overall_arcsec=0.552 sigma_q1_arcsec=0.519 sigma_q2_arcsec=0.624 sigma_q3_arcsec=0.570 sigma_q4_arcsec=0.589 n_q1=2338 n_q2=506 n_q3=1238 n_q4=785 worst_quadrant_to_overall_ratio=1.131
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits -region wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.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-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-39-30_20.00sec_0.00C_LIGHT_0212.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Dra-03-Q2b1x1_004322_TTUQ2b1x1_902118_o1gNgmyQ/wcs_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213.fits
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:40.59 +66:34:29.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:17.07 +65:56:09.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:29.02 +65:52:09.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:29.02 +66:13:59.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:59.76 +66:32:23.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:08.11 +66:41:43.2: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:50:16.57 +70:34:01.0: 13.79 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:20.00 +66:20:35.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:32.01 +66:33:05.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:29.02 +65:52:09.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:40.59 +66:34:29.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:59.76 +66:32:23.4: 13.60 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:29.02 +66:13:59.6: 13.44 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:17.07 +65:56:09.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 11:30:29.02 +65:52:09.0: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3886 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 11:15:59.76 +66:32:23.4: ref_mag=13.66 +/- 0.03 new_mean_mag=12.4698 delta=1.19 (need > 0.90)
Forced photometry filter KEPT candidate at 11:21:40.59 +66:34:29.0: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4052 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 11:30:29.02 +66:13:59.6: ref_mag=13.43 +/- 0.02 new_mean_mag=12.4712 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 11:20:17.07 +65:56:09.8: ref_mag=13.76 +/- 0.03 new_mean_mag=12.6703 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:50:16.57 +70:34:01.0: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:20.00 +66:20:35.7: 13.63 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:31.87 +65:34:40.9: 13.63 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:24:32.01 +66:33:05.8: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:08.11 +66:41:43.2: 13.76 +/- 0.04 detection
Forced photometry filter KEPT candidate at 12:50:16.57 +70:34:01.0: ref_mag=13.76 +/- 0.03 new_mean_mag=12.7591 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 11:22:20.00 +66:20:35.7: ref_mag=13.66 +/- 0.03 new_mean_mag=12.4271 delta=1.23 (need > 0.90)
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 11:24:32.01 +66:33:05.8: ref_mag=13.76 +/- 0.03 new_mean_mag=12.5904 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 11:18:08.11 +66:41:43.2: ref_mag=13.75 +/- 0.03 new_mean_mag=12.5455 delta=1.21 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:31.87 +65:34:40.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 11:28:31.87 +65:34:40.9: ref_mag=13.67 +/- 0.03 new_mean_mag=12.5759 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:53.39 +65:59:49.1: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:53.39 +65:59:49.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 11:19:53.39 +65:59:49.1: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5666 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:36.79 +65:39:24.2: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:41.99 +66:51:27.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:49.56 +65:51:43.6: 13.59 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:25:36.79 +65:39:24.2: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 11:25:36.79 +65:39:24.2: ref_mag=13.61 +/- 0.03 new_mean_mag=12.4272 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:49.52 +65:43:08.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:41.99 +66:51:27.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 11:17:41.99 +66:51:27.0: ref_mag=13.66 +/- 0.03 new_mean_mag=12.6247 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:31:37.02 +65:50:24.0: 13.55 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:49.56 +65:51:43.6: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 11:26:49.56 +65:51:43.6: ref_mag=13.62 +/- 0.03 new_mean_mag=12.4606 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:47.56 +66:58:04.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:42.15 +65:54:29.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:49.52 +65:43:08.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 11:17:49.52 +65:43:08.0: ref_mag=13.59 +/- 0.03 new_mean_mag=12.5127 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:31:37.02 +65:50:24.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 11:31:37.02 +65:50:24.0: ref_mag=13.58 +/- 0.03 new_mean_mag=12.5348 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:47.56 +66:58:04.9: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 11:15:47.56 +66:58:04.9: ref_mag=13.56 +/- 0.03 new_mean_mag=12.5764 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:42.15 +65:54:29.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 11:23:42.15 +65:54:29.5: ref_mag=13.59 +/- 0.03 new_mean_mag=12.3963 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:42.71 +66:24:33.4: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:42.71 +66:24:33.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:42.71 +66:24:33.4: ref_mag=13.51 +/- 0.02 new_mean_mag=12.4160 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:49.50 +66:25:58.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:49.50 +66:25:58.1: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 11:18:49.50 +66:25:58.1: ref_mag=13.54 +/- 0.02 new_mean_mag=12.3717 delta=1.17 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:22.96 +65:45:37.9: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:22.96 +65:45:37.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 11:30:22.96 +65:45:37.9: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4238 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:34.24 +65:21:00.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:54.09 +66:43:05.9: 13.45 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:09.59 +65:38:46.2: 13.39 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:34.24 +65:21:00.1: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 11:18:34.24 +65:21:00.1: ref_mag=13.46 +/- 0.02 new_mean_mag=12.3957 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:44.76 +65:34:05.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:36.37 +65:30:48.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:51.85 +66:18:19.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:54.09 +66:43:05.9: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 11:18:54.09 +66:43:05.9: ref_mag=13.47 +/- 0.03 new_mean_mag=12.4863 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:35:09.59 +65:38:46.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 11:35:09.59 +65:38:46.2: ref_mag=13.42 +/- 0.02 new_mean_mag=12.3937 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:21.58 +66:23:43.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:44.76 +65:34:05.5: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:19:44.76 +65:34:05.5: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3782 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:36.37 +65:30:48.6: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 11:28:36.37 +65:30:48.6: ref_mag=13.39 +/- 0.02 new_mean_mag=12.2698 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:51.85 +66:18:19.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 11:16:51.85 +66:18:19.8: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3780 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:21.58 +66:23:43.7: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 11:21:21.58 +66:23:43.7: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3216 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:39.29 +66:03:20.7: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:39.29 +66:03:20.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 11:30:39.29 +66:03:20.7: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2527 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:24.08 +66:46:38.2: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:24.08 +66:46:38.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:24.08 +66:46:38.2: ref_mag=13.34 +/- 0.02 new_mean_mag=12.2820 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:46.39 +66:21:11.4: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:46.39 +66:21:11.4: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 11:20:46.39 +66:21:11.4: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2941 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:37.39 +66:27:07.6: 13.28 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:15:38.89 +66:35:17.0: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:33.65 +66:38:58.6: 13.29 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:37.39 +66:27:07.6: 13.37 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:15:38.89 +66:35:17.0: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:00.93 +65:42:14.7: 13.27 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:16:37.39 +66:27:07.6: ref_mag=13.33 +/- 0.02 new_mean_mag=12.2204 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 11:15:38.89 +66:35:17.0: ref_mag=13.33 +/- 0.02 new_mean_mag=12.3715 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:53.91 +65:29:51.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:10.50 +66:30:57.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:51.58 +66:21:19.7: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:33.65 +66:38:58.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 11:18:33.65 +66:38:58.6: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2504 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:00.93 +65:42:14.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 11:29:00.93 +65:42:14.7: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2398 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:53.91 +65:29:51.3: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 11:20:53.91 +65:29:51.3: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2502 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:10.50 +66:30:57.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:51.58 +66:21:19.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 11:16:10.50 +66:30:57.9: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2170 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 11:21:51.58 +66:21:19.7: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1512 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:21.24 +65:45:24.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:21.24 +65:45:24.9: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 11:22:21.24 +65:45:24.9: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1589 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:03.09 +66:06:59.0: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:03.09 +66:06:59.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:03.09 +66:06:59.0: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1571 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:01.67 +66:00:04.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:40.96 +66:31:47.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:01.67 +66:00:04.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 11:21:01.67 +66:00:04.4: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1263 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:40.96 +66:31:47.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 11:20:40.96 +66:31:47.4: ref_mag=13.06 +/- 0.02 new_mean_mag=12.1083 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:33:00.60 +65:49:28.0: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:06.93 +65:40:05.5: 13.03 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:00.07 +65:49:06.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:33:00.60 +65:49:28.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 11:33:00.60 +65:49:28.0: ref_mag=13.04 +/- 0.02 new_mean_mag=12.1016 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:06.93 +65:40:05.5: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 11:30:06.93 +65:40:05.5: ref_mag=13.00 +/- 0.02 new_mean_mag=11.9341 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:15.25 +66:10:00.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:00.07 +65:49:06.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 11:22:00.07 +65:49:06.7: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9881 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:29.34 +65:31:23.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:15.25 +66:10:00.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 11:22:15.25 +66:10:00.8: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9731 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:29.34 +65:31:23.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:22:07.88 +65:56:21.0: 12.88 +/- 0.02 detection
Forced photometry filter KEPT candidate at 11:29:29.34 +65:31:23.7: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0022 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:22:07.88 +65:56:21.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 11:22:07.88 +65:56:21.0: ref_mag=12.92 +/- 0.01 new_mean_mag=11.9495 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:08.07 +65:21:59.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:19:08.07 +65:21:59.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 11:19:08.07 +65:21:59.9: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7157 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:26.74 +65:41:49.9: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:31:12.33 +65:49:20.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:24:26.74 +65:41:49.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 11:24:26.74 +65:41:49.9: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8241 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:32:42.51 +65:48:12.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:31:12.33 +65:49:20.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 11:31:12.33 +65:49:20.5: ref_mag=12.78 +/- 0.01 new_mean_mag=11.7947 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:32:42.51 +65:48:12.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 11:32:42.51 +65:48:12.9: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7989 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:21:05.17 +65:38:58.2: 12.72 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:21:05.17 +65:38:58.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 11:21:05.17 +65:38:58.2: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7074 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:45.89 +66:12:47.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:45.89 +66:12:47.6: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 11:16:45.89 +66:12:47.6: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7042 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:55.72 +66:13:12.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:55.72 +66:13:12.6: 12.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 11:18:55.72 +66:13:12.6: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6547 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:27:23.60 +65:47:45.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:27:23.60 +65:47:45.3: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 11:27:23.60 +65:47:45.3: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6910 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:45.49 +65:49:44.3: 12.43 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:20.68 +65:59:01.1: 12.34 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:45.49 +65:49:44.3: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 11:17:45.49 +65:49:44.3: ref_mag=12.44 +/- 0.01 new_mean_mag=11.4694 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:20.68 +65:59:01.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 11:17:20.68 +65:59:01.1: ref_mag=12.36 +/- 0.01 new_mean_mag=11.3813 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:57.79 +65:48:31.8: 12.28 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:57.79 +65:48:31.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 11:18:57.79 +65:48:31.8: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2783 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:28.05 +65:36:26.1: 11.93 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:28.05 +65:36:26.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 11:26:28.05 +65:36:26.1: ref_mag=11.93 +/- 0.01 new_mean_mag=10.9560 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out05421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21083.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 78s
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: 31s
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Considering the candidate 11615_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 11615_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:20:54.15 +67:06:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17232_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 17232_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 12:33:28.20 +69:47:18.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 18099_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 18099_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:31:24.61 +69:19:53.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 10545_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 10545_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:18:46.36 +66:41:02.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 07985_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07985_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10133_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10133_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06664_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06664_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 07198_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 07198_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:28:44.56 +65:57:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08066_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 08066_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10683_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10683_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 21083_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 21083_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09723_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09723_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10966_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10966_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09223_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09223_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06096_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 06096_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:23:15.14 +65:28:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05869_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 05869_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 08342_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 08342_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06470_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06470_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 11599_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 11599_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 23927_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 23927_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:19:05.34 +70:06:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07031_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07031_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06095_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 06095_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:25:35.99 +65:33:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07605_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07605_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06445_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06445_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 07567_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07567_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 12224_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 12224_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10007_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10007_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09953_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09953_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06304_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06304_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06231_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06231_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10934_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10934_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 05421_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 05421_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06814_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06814_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 05644_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 05644_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09760_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09760_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09545_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09545_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 07306_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07306_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 11335_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 11335_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09442_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09442_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10299_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10299_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10880_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10880_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10739_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10739_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06225_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06225_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06427_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06427_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09312_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09312_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10558_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10558_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 07166_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07166_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09033_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09033_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09162_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 09162_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:17:44.87 +66:10:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07319_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 07319_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:18:45.09 +65:40:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08225_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 08225_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 10070_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 10070_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 08032_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 08032_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:21:33.97 +65:58:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06244_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06244_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06009_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06009_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 08011_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 08011_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:23:33.70 +66:01:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07418_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07418_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 08605_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 08605_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 05572_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 05572_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06083_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 06083_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:26:09.36 +65:34:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07833_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07833_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06176_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06176_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06712_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06712_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06408_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06408_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06208_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06208_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 06941_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06941_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 09417_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09417_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09167_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 09167_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06710_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06710_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07480_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 07480_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:20:55.96 +65:48:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07206_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 07206_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:20:09.36 +65:42:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07983_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07983_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08544_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 08544_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07734_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 07734_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06115_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 06115_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07094_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 07094_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 11:21:21.85 +65:42:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14729_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 14729_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 12:30:05.87 +69:12:03.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18196_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213
The candidate 18196_fd_Dra-03-Q2b1x1_2026-08-06_00-40-31_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 12:34:43.35 +70:01:19.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 113s
Prepared the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:35:09.59 +65:38:46.2
11:29:29.34 +65:31:23.7
11:28:36.37 +65:30:48.6
11:28:31.87 +65:34:40.9
11:30:06.93 +65:40:05.5
11:26:28.05 +65:36:26.1
11:19:08.07 +65:21:59.9
11:32:42.51 +65:48:12.9
11:29:00.93 +65:42:14.7
11:18:34.24 +65:21:00.1
11:33:00.60 +65:49:28.0
11:30:22.96 +65:45:37.9
11:31:12.33 +65:49:20.5
11:20:53.91 +65:29:51.3
11:31:37.02 +65:50:24.0
11:25:36.79 +65:39:24.2
11:30:29.02 +65:52:09.0
11:27:23.60 +65:47:45.3
11:24:26.74 +65:41:49.9
11:19:44.76 +65:34:05.5
11:21:05.17 +65:38:58.2
11:26:49.56 +65:51:43.6
11:22:21.24 +65:45:24.9
11:30:39.29 +66:03:20.7
11:22:00.07 +65:49:06.7
11:23:42.15 +65:54:29.5
11:17:49.52 +65:43:08.0
11:18:57.79 +65:48:31.8
11:22:07.88 +65:56:21.0
11:17:45.49 +65:49:44.3
11:30:29.02 +66:13:59.6
11:20:17.07 +65:56:09.8
11:21:01.67 +66:00:04.4
11:19:53.39 +65:59:49.1
11:17:20.68 +65:59:01.1
11:22:15.25 +66:10:00.8
11:17:03.09 +66:06:59.0
11:18:55.72 +66:13:12.6
11:22:20.00 +66:20:35.7
11:21:51.58 +66:21:19.7
11:16:45.89 +66:12:47.6
11:20:46.39 +66:21:11.4
11:21:21.58 +66:23:43.7
11:24:32.01 +66:33:05.8
11:16:51.85 +66:18:19.8
11:18:49.50 +66:25:58.1
11:17:42.71 +66:24:33.4
11:20:40.96 +66:31:47.4
11:21:40.59 +66:34:29.0
11:16:37.39 +66:27:07.6
11:16:10.50 +66:30:57.9
11:15:59.76 +66:32:23.4
11:18:33.65 +66:38:58.6
11:15:38.89 +66:35:17.0
11:18:54.09 +66:43:05.9
11:18:08.11 +66:41:43.2
11:17:24.08 +66:46:38.2
11:17:41.99 +66:51:27.0
11:15:47.56 +66:58:04.9
12:50:16.57 +70:34:01.0
########### Completed Dra-03-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 ####
11:30:29.02 +66:13:59.6
11:21:40.59 +66:34:29.0
11:30:29.02 +65:52:09.0
11:20:17.07 +65:56:09.8
11:15:59.76 +66:32:23.4
12:50:16.57 +70:34:01.0
11:24:32.01 +66:33:05.8
11:18:08.11 +66:41:43.2
11:22:20.00 +66:20:35.7
11:28:31.87 +65:34:40.9
11:19:53.39 +65:59:49.1
11:25:36.79 +65:39:24.2
11:17:41.99 +66:51:27.0
11:26:49.56 +65:51:43.6
11:17:49.52 +65:43:08.0
11:31:37.02 +65:50:24.0
11:23:42.15 +65:54:29.5
11:15:47.56 +66:58:04.9
11:17:42.71 +66:24:33.4
11:18:49.50 +66:25:58.1
11:30:22.96 +65:45:37.9
11:18:34.24 +65:21:00.1
11:18:54.09 +66:43:05.9
11:35:09.59 +65:38:46.2
11:19:44.76 +65:34:05.5
11:28:36.37 +65:30:48.6
11:16:51.85 +66:18:19.8
11:21:21.58 +66:23:43.7
11:30:39.29 +66:03:20.7
11:17:24.08 +66:46:38.2
11:20:46.39 +66:21:11.4
11:16:37.39 +66:27:07.6
11:15:38.89 +66:35:17.0
11:18:33.65 +66:38:58.6
11:29:00.93 +65:42:14.7
11:20:53.91 +65:29:51.3
11:21:51.58 +66:21:19.7
11:16:10.50 +66:30:57.9
11:22:21.24 +65:45:24.9
11:17:03.09 +66:06:59.0
11:21:01.67 +66:00:04.4
11:20:40.96 +66:31:47.4
11:33:00.60 +65:49:28.0
11:30:06.93 +65:40:05.5
11:22:00.07 +65:49:06.7
11:22:15.25 +66:10:00.8
11:29:29.34 +65:31:23.7
11:22:07.88 +65:56:21.0
11:19:08.07 +65:21:59.9
11:24:26.74 +65:41:49.9
11:31:12.33 +65:49:20.5
11:32:42.51 +65:48:12.9
11:21:05.17 +65:38:58.2
11:16:45.89 +66:12:47.6
11:18:55.72 +66:13:12.6
11:27:23.60 +65:47:45.3
11:17:45.49 +65:49:44.3
11:17:20.68 +65:59:01.1
11:18:57.79 +65:48:31.8
11:26:28.05 +65:36:26.1
###################################################################################
11:30:29.02 +66:13:59.6 -- not an asteroid (will add it to exclusion list)
11:21:40.59 +66:34:29.0 -- not an asteroid (will add it to exclusion list)
11:30:29.02 +65:52:09.0 -- not an asteroid (will add it to exclusion list)
11:20:17.07 +65:56:09.8 -- not an asteroid (will add it to exclusion list)
11:15:59.76 +66:32:23.4 -- not an asteroid (will add it to exclusion list)
12:50:16.57 +70:34:01.0 -- not an asteroid (will add it to exclusion list)
11:24:32.01 +66:33:05.8 -- not an asteroid (will add it to exclusion list)
11:18:08.11 +66:41:43.2 -- not an asteroid (will add it to exclusion list)
11:22:20.00 +66:20:35.7 -- not an asteroid (will add it to exclusion list)
11:28:31.87 +65:34:40.9 -- not an asteroid (will add it to exclusion list)
11:19:53.39 +65:59:49.1 -- not an asteroid (will add it to exclusion list)
11:25:36.79 +65:39:24.2 -- not an asteroid (will add it to exclusion list)
11:17:41.99 +66:51:27.0 -- not an asteroid (will add it to exclusion list)
11:26:49.56 +65:51:43.6 -- not an asteroid (will add it to exclusion list)
11:17:49.52 +65:43:08.0 -- not an asteroid (will add it to exclusion list)
11:31:37.02 +65:50:24.0 -- not an asteroid (will add it to exclusion list)
11:23:42.15 +65:54:29.5 -- not an asteroid (will add it to exclusion list)
11:15:47.56 +66:58:04.9 -- not an asteroid (will add it to exclusion list)
11:17:42.71 +66:24:33.4 -- not an asteroid (will add it to exclusion list)
11:18:49.50 +66:25:58.1 -- not an asteroid (will add it to exclusion list)
11:30:22.96 +65:45:37.9 -- not an asteroid (will add it to exclusion list)
11:18:34.24 +65:21:00.1 -- not an asteroid (will add it to exclusion list)
11:18:54.09 +66:43:05.9 -- not an asteroid (will add it to exclusion list)
11:35:09.59 +65:38:46.2 -- not an asteroid (will add it to exclusion list)
11:19:44.76 +65:34:05.5 -- not an asteroid (will add it to exclusion list)
11:28:36.37 +65:30:48.6 -- not an asteroid (will add it to exclusion list)
11:16:51.85 +66:18:19.8 -- not an asteroid (will add it to exclusion list)
11:21:21.58 +66:23:43.7 -- not an asteroid (will add it to exclusion list)
11:30:39.29 +66:03:20.7 -- not an asteroid (will add it to exclusion list)
11:17:24.08 +66:46:38.2 -- not an asteroid (will add it to exclusion list)
11:20:46.39 +66:21:11.4 -- not an asteroid (will add it to exclusion list)
11:16:37.39 +66:27:07.6 -- not an asteroid (will add it to exclusion list)
11:15:38.89 +66:35:17.0 -- not an asteroid (will add it to exclusion list)
11:18:33.65 +66:38:58.6 -- not an asteroid (will add it to exclusion list)
11:29:00.93 +65:42:14.7 -- not an asteroid (will add it to exclusion list)
11:20:53.91 +65:29:51.3 -- not an asteroid (will add it to exclusion list)
11:21:51.58 +66:21:19.7 -- not an asteroid (will add it to exclusion list)
11:16:10.50 +66:30:57.9 -- not an asteroid (will add it to exclusion list)
11:22:21.24 +65:45:24.9 -- not an asteroid (will add it to exclusion list)
11:17:03.09 +66:06:59.0 -- not an asteroid (will add it to exclusion list)
11:21:01.67 +66:00:04.4 -- not an asteroid (will add it to exclusion list)
11:20:40.96 +66:31:47.4 -- not an asteroid (will add it to exclusion list)
11:33:00.60 +65:49:28.0 -- not an asteroid (will add it to exclusion list)
11:30:06.93 +65:40:05.5 -- not an asteroid (will add it to exclusion list)
11:22:00.07 +65:49:06.7 -- not an asteroid (will add it to exclusion list)
11:22:15.25 +66:10:00.8 -- not an asteroid (will add it to exclusion list)
11:29:29.34 +65:31:23.7 -- not an asteroid (will add it to exclusion list)
11:22:07.88 +65:56:21.0 -- not an asteroid (will add it to exclusion list)
11:19:08.07 +65:21:59.9 -- not an asteroid (will add it to exclusion list)
11:24:26.74 +65:41:49.9 -- not an asteroid (will add it to exclusion list)
11:31:12.33 +65:49:20.5 -- not an asteroid (will add it to exclusion list)
11:32:42.51 +65:48:12.9 -- not an asteroid (will add it to exclusion list)
11:21:05.17 +65:38:58.2 -- not an asteroid (will add it to exclusion list)
11:16:45.89 +66:12:47.6 -- not an asteroid (will add it to exclusion list)
11:18:55.72 +66:13:12.6 -- not an asteroid (will add it to exclusion list)
11:27:23.60 +65:47:45.3 -- not an asteroid (will add it to exclusion list)
11:17:45.49 +65:49:44.3 -- not an asteroid (will add it to exclusion list)
11:17:20.68 +65:59:01.1 -- not an asteroid (will add it to exclusion list)
11:18:57.79 +65:48:31.8 -- not an asteroid (will add it to exclusion list)
11:26:28.05 +65:36:26.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:15:38.89 +66:35:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:15:47.56 +66:58:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:15:59.76 +66:32:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:10.50 +66:30:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:37.39 +66:27:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:45.89 +66:12:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:51.85 +66:18:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:03.09 +66:06:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:20.68 +65:59:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:24.08 +66:46:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:41.99 +66:51:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:42.71 +66:24:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:45.49 +65:49:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:49.52 +65:43:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:08.11 +66:41:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:33.65 +66:38:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:34.24 +65:21:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:49.50 +66:25:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:54.09 +66:43:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:55.72 +66:13:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:57.79 +65:48:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:08.07 +65:21:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:44.76 +65:34:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:53.39 +65:59:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:17.07 +65:56:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:40.96 +66:31:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:46.39 +66:21:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:53.91 +65:29:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:01.67 +66:00:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:05.17 +65:38:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:21.58 +66:23:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:40.59 +66:34:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:51.58 +66:21:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:22:00.07 +65:49:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:22:07.88 +65:56:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:22:15.25 +66:10:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:22:20.00 +66:20:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:22:21.24 +65:45:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:23:42.15 +65:54:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:24:26.74 +65:41:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:24:32.01 +66:33:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:25:36.79 +65:39:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:28.05 +65:36:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:49.56 +65:51:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:27:23.60 +65:47:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:31.87 +65:34:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:36.37 +65:30:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:00.93 +65:42:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:29.34 +65:31:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:06.93 +65:40:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:22.96 +65:45:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:29.02 +65:52:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:29.02 +66:13:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:39.29 +66:03:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:31:12.33 +65:49:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:31:37.02 +65:50:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:32:42.51 +65:48:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:33:00.60 +65:49:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:09.59 +65:38:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:16.57 +70:34:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:15:38.89 +66:35:17.0 -- not a known variable star
11:15:47.56 +66:58:04.9 -- not a known variable star
11:15:59.76 +66:32:23.4 -- not a known variable star
11:16:10.50 +66:30:57.9 -- not a known variable star
11:16:37.39 +66:27:07.6 -- a known variable star
11:16:45.89 +66:12:47.6 -- not a known variable star
11:16:51.85 +66:18:19.8 -- not a known variable star
11:17:03.09 +66:06:59.0 -- not a known variable star
11:17:20.68 +65:59:01.1 -- not a known variable star
11:17:24.08 +66:46:38.2 -- not a known variable star
11:17:41.99 +66:51:27.0 -- not a known variable star
11:17:42.71 +66:24:33.4 -- not a known variable star
11:17:45.49 +65:49:44.3 -- not a known variable star
11:17:49.52 +65:43:08.0 -- not a known variable star
11:18:08.11 +66:41:43.2 -- not a known variable star
11:18:33.65 +66:38:58.6 -- not a known variable star
11:18:34.24 +65:21:00.1 -- not a known variable star
11:18:49.50 +66:25:58.1 -- not a known variable star
11:18:54.09 +66:43:05.9 -- not a known variable star
11:18:55.72 +66:13:12.6 -- a known variable star
11:18:57.79 +65:48:31.8 -- not a known variable star
11:19:08.07 +65:21:59.9 -- a known variable star
11:19:44.76 +65:34:05.5 -- not a known variable star
11:19:53.39 +65:59:49.1 -- not a known variable star
11:20:17.07 +65:56:09.8 -- not a known variable star
11:20:40.96 +66:31:47.4 -- not a known variable star
11:20:46.39 +66:21:11.4 -- not a known variable star
11:20:53.91 +65:29:51.3 -- not a known variable star
11:21:01.67 +66:00:04.4 -- not a known variable star
11:21:05.17 +65:38:58.2 -- not a known variable star
11:21:21.58 +66:23:43.7 -- not a known variable star
11:21:40.59 +66:34:29.0 -- not a known variable star
11:21:51.58 +66:21:19.7 -- not a known variable star
11:22:00.07 +65:49:06.7 -- not a known variable star
11:22:07.88 +65:56:21.0 -- not a known variable star
11:22:15.25 +66:10:00.8 -- not a known variable star
11:22:20.00 +66:20:35.7 -- not a known variable star
11:22:21.24 +65:45:24.9 -- not a known variable star
11:23:42.15 +65:54:29.5 -- not a known variable star
11:24:26.74 +65:41:49.9 -- a known variable star
11:24:32.01 +66:33:05.8 -- a known variable star
11:25:36.79 +65:39:24.2 -- not a known variable star
11:26:28.05 +65:36:26.1 -- not a known variable star
11:26:49.56 +65:51:43.6 -- not a known variable star
11:27:23.60 +65:47:45.3 -- not a known variable star
11:28:31.87 +65:34:40.9 -- not a known variable star
11:28:36.37 +65:30:48.6 -- not a known variable star
11:29:00.93 +65:42:14.7 -- not a known variable star
11:29:29.34 +65:31:23.7 -- not a known variable star
11:30:06.93 +65:40:05.5 -- not a known variable star
11:30:22.96 +65:45:37.9 -- not a known variable star
11:30:29.02 +65:52:09.0 -- not a known variable star
11:30:29.02 +66:13:59.6 -- not a known variable star
11:30:39.29 +66:03:20.7 -- not a known variable star
11:31:12.33 +65:49:20.5 -- not a known variable star
11:31:37.02 +65:50:24.0 -- not a known variable star
11:32:42.51 +65:48:12.9 -- not a known variable star
11:33:00.60 +65:49:28.0 -- not a known variable star
11:35:09.59 +65:38:46.2 -- not a known variable star
12:50:16.57 +70:34:01.0 -- not a known variable star
Found 55 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
60 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 60 (excluding asteroids and hot pixels, 55 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.73588348 -observatory V36
07:45:43.40 +20:23:15.8 Mercury (-0.3mag)
11:55:44.63 -00:04:29.1 Venus (-4.3mag)
05:43:29.28 +23:32:41.6 Mars (1.3mag)
08:41:09.02 +18:47:54.9 Jupiter (-1.8mag)
00:56:32.91 +03:16:46.4 Saturn (0.6mag)
04:11:29.83 +20:56:20.9 Uranus (5.8mag)
00:16:12.74 +00:13:58.4 Neptune (7.7mag)
20:28:19.91 -23:29:24.6 Pluto (14.4mag)
02:48:01.09 +20:41:42.3 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 00:45 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461258.73588348:
08:41:15.76 +18:47:26.2 Io (6.0mag)
08:41:05.51 +18:48:10.5 Europa (6.3mag)
08:41:05.77 +18:48:12.8 Ganymede (5.6mag)
08:40:55.42 +18:48:56.1 Callisto (6.7mag)
08:38:44.89 +18:46:05.4 Himalia (15.7mag)
08:41:07.13 +18:48:03.7 Thebe (16.6mag)
08:38:15.54 +18:45:00.5 Elara (17.7mag)
08:45:14.93 +18:28:19.1 Pasiphae (17.9mag)
08:44:27.77 +18:57:45.5 Carme (19.0mag)
00:56:30.59 +03:17:13.4 Titan (8.4mag)
00:56:27.14 +03:16:49.9 Rhea (9.7mag)
00:56:36.59 +03:15:08.8 Iapetus (11.1mag)
00:56:19.47 +03:17:00.6 Hyperion (14.4mag)
00:55:57.93 +03:10:13.0 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 00:45 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.73588348:
18:55:34.23 -24:03:01.3 JWST
17:14:34.77 +41:23:53.1 Chandra
09:32:50.40 -53:53:18.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 00:45 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.73588348 -observatory V36
03:11:24.37 +17:12:31.7 17.7mag P/1996 R2 (Lagerkvist)
18:02:24.24 -34:38:23.6 14.0mag P/2010 H2 (Vales)
06:51:55.85 -68:49:41.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:17.29 +32:57:06.4 17.7mag C/2017 K2 (PANSTARRS)
03:37:45.92 +36:44:21.0 16.7mag P/2021 N1 (ZTF)
22:40:16.02 +31:33:53.2 17.3mag C/2022 E2 (ATLAS)
06:41:29.77 +26:34:30.6 16.8mag C/2022 N2 (PANSTARRS)
10:19:43.77 +28:33:32.7 17.0mag C/2022 QE78 (ATLAS)
09:27:31.66 +05:17:43.6 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.30 -12:12:30.5 17.9mag P/2023 B1 (PANSTARRS)
21:13:23.89 +66:13:49.7 17.9mag C/2023 H5 (Lemmon)
15:49:53.39 -12:45:01.2 14.3mag C/2023 R1 (PANSTARRS)
08:05:51.16 +31:15:22.9 15.2mag C/2024 E1 (Wierzchos)
15:07:17.61 +15:36:58.5 17.7mag C/2024 G6 (ATLAS)
19:05:39.31 +42:57:45.5 13.7mag C/2024 J3 (ATLAS)
21:13:38.89 +49:04:46.2 17.6mag C/2024 R4 (PANSTARRS)
05:13:32.04 -12:59:37.6 15.5mag C/2024 T5 (ATLAS)
06:54:55.46 +24:30:20.3 17.9mag C/2025 J1 (Borisov)
07:29:57.30 -15:52:07.4 17.7mag C/2025 R3 (PANSTARRS)
10:30:08.63 +21:01:49.2 17.3mag C/2025 V2 (Rankin)
12:56:56.88 +02:28:52.4 17.0mag C/2025 Y1 (ATLAS)
16:03:41.65 +78:01:02.3 16.8mag C/2026 A2 (Bok)
03:06:43.35 +46:08:44.0 17.1mag C/2026 B2 (Sun-Gao)
11:45:09.46 +08:20:02.2 17.3mag A/2026 E1
21:56:07.76 -26:27:42.8 6.9mag 10P/Tempel
11:27:46.47 -03:16:38.0 16.2mag 29P/Schwassmann-Wachmann
04:36:46.37 +32:15:47.7 18.0mag 47P/Ashbrook-Jackson
11:03:38.02 +05:17:33.3 17.2mag 63P/Wild
00:54:17.91 -05:22:44.2 15.4mag 65P/Gunn
05:31:01.78 +20:43:45.9 13.7mag 78P/Gehrels
20:39:46.82 -23:17:37.0 17.8mag 84P/Giclas
02:58:44.26 +13:32:26.4 16.7mag 88P/Howell
07:50:47.66 +27:55:36.7 16.1mag 93P/Lovas
04:00:45.96 +16:06:04.6 17.6mag 112P/Urata-Niijima
05:49:54.53 +30:30:48.8 16.3mag 114P/Wiseman-Skiff
09:13:46.57 +26:59:02.5 15.0mag 123P/West-Hartley
11:39:45.48 -09:30:10.8 17.1mag 124P/Mrkos
05:33:36.92 +21:11:10.5 16.1mag 128P/Shoemaker-Holt
06:25:06.31 +18:59:44.1 17.9mag 131P/Mueller
00:03:41.74 +03:25:21.4 17.6mag 139P/Vaisala-Oterma
03:21:33.93 -19:44:52.6 14.0mag 161P/Hartley-IRAS
07:09:16.85 +37:41:26.0 15.8mag 162P/SidingSpring
15:49:43.48 +39:30:10.1 12.3mag 169P/NEAT
02:39:19.76 +09:28:32.8 17.6mag 220P/McNaught
16:40:35.65 -09:56:43.1 17.6mag 235P/LINEAR
20:23:43.40 -52:50:56.2 17.8mag 259P/Garradd
03:16:19.19 +24:19:29.5 15.4mag 260P/McNaught
06:59:22.37 +37:45:16.4 17.3mag 295P/LINEAR
15:09:51.18 +03:21:27.4 17.7mag 391P/Kowalski
08:59:04.33 +18:28:24.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 00:45 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 00:45 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 00:45 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
18:14:11.533 +25:31:50.45 AT 2026vkg 2026-07-16.29 20.95
22:50:03.729 +40:38:42.44 AT 2026vkf 2026-07-20.53 20.32
-rw-r--r-- 1 apache apache 87K Aug 6 00:45 tns_transients_list.txt
