This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.92 13:26:41.19 +69:58:38.4
118.53338 46.84873 galactic UMi Second-epoch detections are separated by 2.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:41.19 +69:58:38.4 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:26:41.19 +69:58:38.4: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:26:41.19 +69:58:38.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461231.7332,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.10 10:34:01.29 +68:57:59.3
139.16636 43.57566 galactic UMa Second-epoch detections are separated by 1.6" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:34:01.29 +68:57:59.3 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:01.29 +68:57:59.3: 13.06 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:34:01.29 +68:57:59.3: 13.01 +/- 0.03 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!
TCP 2026 07 10.2332* 10 34 01.29 +68 57 59.3 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,2461231.7332,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.01 13:01:50.82 +72:20:36.1
121.82059 44.76242 galactic Dra Second-epoch detections are separated by 0.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:50.82 +72:20:36.1 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:50.82 +72:20:36.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:50.82 +72:20:36.1: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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,2461231.7332,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.62 13:15:38.77 +73:42:31.5
120.60247 43.30984 galactic UMi Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:38.77 +73:42:31.5 (user input) | T | P | (position from user input) J-Ks=0.592+/-0.037 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:38.77 +73:42:31.5: 13.75 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:38.77 +73:42:31.5: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.46 13:03:29.52 +72:40:30.8
121.67587 44.42362 galactic Dra Second-epoch detections are separated by 1.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:03:29.52 +72:40:30.8 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:03:29.52 +72:40:30.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:03:29.52 +72:40:30.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.46 13:11:09.51 +72:58:11.6
120.92395 44.08139 galactic UMi Second-epoch detections are separated by 1.3" and 2.5 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 | 13:11:09.51 +72:58:11.6 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.035 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:09.51 +72:58:11.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:09.51 +72:58:11.6: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.48 13:19:34.04 +73:17:51.8
120.14331 43.67790 galactic UMi Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:34.04 +73:17:51.8 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.035 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:34.04 +73:17:51.8: 13.62 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:34.04 +73:17:51.8: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 11.76 13:27:03.14 +69:12:18.1
118.25789 47.59871 galactic Dra Second-epoch detections are separated by 1.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1685230718957990784 | 13:27:03.13 +69:12:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:27:03.14 +69:12:18.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:27:03.14 +69:12:18.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1685230718957990784,2461231.7332,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1685230718957990784 20260710.2332 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.60 13:09:38.14 +72:43:43.4
121.04523 44.33280 galactic UMi Second-epoch detections are separated by 0.6" and 2.4 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 | 13:09:38.14 +72:43:43.4 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.036 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:09:38.14 +72:43:43.4: 13.60 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:09:38.14 +72:43:43.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.26 13:13:09.40 +72:57:01.0
120.71839 44.08451 galactic UMi Second-epoch detections are separated by 4.1" and 2.5 pix
The object was found in VSX 0" Gaia DR3 1688175520334678016
Type: ROT
# Max. Min./Amp. JD0 Period
13.170 G 13.210 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:09.40 +72:57:01.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:09.40 +72:57:01.0: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688175520334678016,2461231.7332,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688175520334678016 20260710.2332 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.23 13:11:46.07 +72:34:36.4
120.80176 44.46729 galactic UMi Second-epoch detections are separated by 1.2" and 2.5 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 | 13:11:46.07 +72:34:36.4 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:46.07 +72:34:36.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:46.07 +72:34:36.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.30 13:19:11.71 +73:25:37.5
120.20641 43.55397 galactic UMi Second-epoch detections are separated by 1.7" and 2.4 pix
The object was found in VSX 0" ASASSN-V J131911.67+732537.2
Type: ROT
# Max. Min./Amp. JD0 Period
13.910 g Y 0.220 g 2459400.84800 1.000400000000
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:11.71 +73:25:37.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:11.71 +73:25:37.5: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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
ASASSN-V J131911.67+732537.2,2461231.7332,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J131911.67+732537.2 20260710.2332 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.12 11:10:15.05 +68:32:04.6
135.93024 45.95607 galactic UMa Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:10:15.05 +68:32:04.6 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:10:15.05 +68:32:04.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:10:15.05 +68:32:04.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 11 10 15.05 +68 32 04.6 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,2461231.7332,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.20 13:33:45.63 +72:36:21.5
118.54367 44.15988 galactic UMi Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:33:45.63 +72:36:21.5 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.034 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:33:45.63 +72:36:21.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:33:45.63 +72:36:21.5: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.03 10:41:39.19 +67:34:15.8
139.78220 45.07620 galactic UMa Second-epoch detections are separated by 1.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:41:39.19 +67:34:15.8 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:39.19 +67:34:15.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:41:39.19 +67:34:15.8: 12.98 +/- 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 07 10.2332* 10 41 39.19 +67 34 15.8 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,2461231.7332,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.71 12:56:45.03 +72:15:19.7
122.36084 44.86689 galactic Dra Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689596428659556224 | 12:56:45.05 +72:15:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.025 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:56:45.03 +72:15:19.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:56:45.03 +72:15:19.7: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689596428659556224,2461231.7332,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689596428659556224 20260710.2332 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 07 10.2332 2461231.7332 12.36 13:11:09.60 +72:48:42.3
120.90030 44.23862 galactic UMi Second-epoch detections are separated by 1.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:09.60 +72:48:42.3 (user input) | T | P | (position from user input) J-Ks=0.636+/-0.036 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:09.60 +72:48:42.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:09.60 +72:48:42.3: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.61 13:13:55.43 +72:54:06.5
120.63248 44.12591 galactic UMi Second-epoch detections are separated by 1.3" and 2.5 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 | Gaia DR3 1688163421410823552 | 13:13:55.54 +72:54:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.032 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:55.43 +72:54:06.5: 12.56 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:55.43 +72:54:06.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688163421410823552,2461231.7332,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688163421410823552 20260710.2332 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.19 13:19:46.85 +73:20:22.3
120.13111 43.63426 galactic UMi Second-epoch detections are separated by 0.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1688389787663037056 | 13:19:46.85 +73:20:22.3 (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=0.448+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:46.85 +73:20:22.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:46.85 +73:20:22.3: 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!
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 1688389787663037056,2461231.7332,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1688389787663037056 20260710.2332 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.12 13:15:55.52 +73:00:02.8
120.44741 44.00915 galactic UMi Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:55.52 +73:00:02.8 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.039 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:55.52 +73:00:02.8: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:55.52 +73:00:02.8: 13.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.51 13:10:14.06 +73:53:08.4
121.14511 43.17731 galactic UMi Second-epoch detections are separated by 4.0" and 2.8 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 | 13:10:14.06 +73:53:08.4 (user input) | T | P | (position from user input) J-Ks=0.514+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:10:14.06 +73:53:08.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:10:14.06 +73:53:08.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.41 13:11:30.58 +72:57:37.3
120.88693 44.08810 galactic UMi Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:30.58 +72:57:37.3 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:30.58 +72:57:37.3: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:30.58 +72:57:37.3: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.93 13:12:35.16 +72:59:47.9
120.78360 44.04329 galactic UMi Second-epoch detections are separated by 0.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:35.16 +72:59:47.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:35.16 +72:59:47.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:35.16 +72:59:47.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.96 13:21:06.13 +73:48:02.9
120.10221 43.16408 galactic UMi Second-epoch detections are separated by 1.6" and 2.6 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 | 13:21:06.13 +73:48:02.9 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:21:06.13 +73:48:02.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:21:06.13 +73:48:02.9: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461231.7332,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 11.97 13:01:01.20 +72:35:11.1
121.92664 44.52313 galactic Dra Second-epoch detections are separated by 0.9" and 2.4 pix
The object was found in VSX 7" Gaia DR3 1688108106527911680
Type: ROT
# Max. Min./Amp. JD0 Period
12.320 G 12.350 G M
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:01.20 +72:35:11.1: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:01.20 +72:35:11.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688108106527911680,2461231.7332,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688108106527911680 20260710.2332 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 07 10.2332 2461231.7332 12.54 12:58:13.84 +72:38:48.1
122.22220 44.47220 galactic Dra Second-epoch detections are separated by 3.5" and 2.5 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 | 12:58:13.84 +72:38:48.1 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:13.84 +72:38:48.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:13.84 +72:38:48.1: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.93 13:20:11.43 +73:26:09.2
120.11147 43.53455 galactic UMi Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:11.43 +73:26:09.2 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:20:11.43 +73:26:09.2: 12.93 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:20:11.43 +73:26:09.2: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.01 13:02:07.69 +71:56:19.7
121.75708 45.16505 galactic Dra Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:02:07.69 +71:56:19.7 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:02:07.69 +71:56:19.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:02:07.69 +71:56:19.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461231.7332,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 11.98 10:38:16.62 +68:02:21.6
139.66224 44.51612 galactic UMa Second-epoch detections are separated by 0.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:38:16.62 +68:02:21.6 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:38:16.62 +68:02:21.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:38:16.62 +68:02:21.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 10 38 16.62 +68 02 21.6 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,2461231.7332,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.04 13:15:43.56 +73:10:10.7
120.49813 43.84365 galactic UMi Second-epoch detections are separated by 1.1" and 2.5 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 | 13:15:43.56 +73:10:10.7 (user input) | T | P | (position from user input) J-Ks=0.688+/-0.035 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:43.56 +73:10:10.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:43.56 +73:10:10.7: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.13 10:36:16.71 +68:14:23.5
139.65810 44.24261 galactic UMa Second-epoch detections are separated by 3.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:36:16.71 +68:14:23.5 (user input) | T | P | (position from user input) J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:16.71 +68:14:23.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:36:16.71 +68:14:23.5: 13.17 +/- 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 07 10.2332* 10 36 16.71 +68 14 23.5 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,2461231.7332,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.42 13:13:18.51 +73:18:18.9
120.76100 43.73069 galactic UMi Second-epoch detections are separated by 3.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:18.51 +73:18:18.9 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.037 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:18.51 +73:18:18.9: 13.35 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:18.51 +73:18:18.9: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.19 13:14:08.49 +72:32:32.2
120.54857 44.48076 galactic UMi Second-epoch detections are separated by 1.3" and 2.5 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 | 13:14:08.49 +72:32:32.2 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.035 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:08.49 +72:32:32.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:08.49 +72:32:32.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.54 13:14:27.75 +73:56:33.9
120.75496 43.08804 galactic UMi Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:27.75 +73:56:33.9 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:27.75 +73:56:33.9: 13.76 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:27.75 +73:56:33.9: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.49 13:15:00.24 +73:47:23.9
120.67786 43.23499 galactic UMi Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:00.24 +73:47:23.9 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.034 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:00.24 +73:47:23.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:00.24 +73:47:23.9: 13.64 +/- 0.05 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,2461231.7332,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.01 13:23:25.77 +71:20:57.4
119.28880 45.55200 galactic UMi Second-epoch detections are separated by 0.6" and 2.5 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 | 13:23:25.77 +71:20:57.4 (user input) | T | P | (position from user input) J-Ks=0.569+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:23:25.77 +71:20:57.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:23:25.77 +71:20:57.4: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461231.7332,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.02 12:58:03.43 +72:40:46.9
122.24199 44.43969 galactic Dra Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:03.43 +72:40:46.9 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:03.43 +72:40:46.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:03.43 +72:40:46.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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,2461231.7332,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.55 13:12:26.52 +72:59:51.6
120.79832 44.04347 galactic UMi Second-epoch detections are separated by 1.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:26.52 +72:59:51.6 (user input) | T | P | (position from user input) J-Ks=0.324+/-0.035 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:26.52 +72:59:51.6: 13.71 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:26.52 +72:59:51.6: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.45 13:16:23.22 +73:16:26.1
120.45173 43.73399 galactic UMi Second-epoch detections are separated by 1.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:23.22 +73:16:26.1 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.038 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:16:23.22 +73:16:26.1: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:16:23.22 +73:16:26.1: 13.65 +/- 0.05 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,2461231.7332,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.97 13:13:07.81 +73:49:12.6
120.86086 43.22075 galactic UMi Second-epoch detections are separated by 0.5" and 2.4 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 | 13:13:07.81 +73:49:12.6 (user input) | T | P | (position from user input) J-Ks=0.309+/- (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:07.81 +73:49:12.6: 12.91 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:07.81 +73:49:12.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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,2461231.7332,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 11.95 13:14:32.95 +72:41:52.7
120.53338 44.32249 galactic UMi Second-epoch detections are separated by 2.3" and 2.6 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 | 13:14:32.95 +72:41:52.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.038 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:32.95 +72:41:52.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:32.95 +72:41:52.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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,2461231.7332,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.54 13:15:39.99 +73:30:53.6
120.56603 43.50189 galactic UMi Second-epoch detections are separated by 1.3" and 2.5 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 | Large-amplitude variable Gaia DR2 1688588971066432128 | 13:15:39.99 +73:30:53.6 (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=0.886+/-0.031 (M)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:39.99 +73:30:53.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:39.99 +73:30:53.6: 13.63 +/- 0.05 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!
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 1688588971066432128,2461231.7332,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1688588971066432128 20260710.2332 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.19 13:22:47.96 +73:44:58.3
119.93039 43.19547 galactic UMi Second-epoch detections are separated by 1.8" and 2.6 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 | 13:22:47.96 +73:44:58.3 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:22:47.96 +73:44:58.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:22:47.96 +73:44:58.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.88 10:40:26.28 +67:31:06.6
139.95333 45.03603 galactic UMa Second-epoch detections are separated by 4.2" and 1.6 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 | 10:40:26.28 +67:31:06.6 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:40:26.28 +67:31:06.6: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:40:26.28 +67:31:06.6: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 10 40 26.28 +67 31 06.6 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,2461231.7332,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.93 13:18:25.42 +73:11:59.8
120.23611 43.78678 galactic UMi Second-epoch detections are separated by 0.5" and 2.4 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 | 13:18:25.42 +73:11:59.8 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:18:25.42 +73:11:59.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:18:25.42 +73:11:59.8: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461231.7332,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.88 13:22:31.96 +73:39:29.4
119.93490 43.28867 galactic UMi Second-epoch detections are separated by 0.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:31.96 +73:39:29.4 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:22:31.96 +73:39:29.4: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:22:31.96 +73:39:29.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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,2461231.7332,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.91 12:58:19.78 +72:16:20.8
122.19207 44.84591 galactic Dra Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:19.78 +72:16:20.8 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:19.78 +72:16:20.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:19.78 +72:16:20.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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,2461231.7332,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.24 12:57:55.37 +72:12:02.2
122.23212 44.91883 galactic Dra Second-epoch detections are separated by 3.3" and 2.5 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 | 12:57:55.37 +72:12:02.2 (user input) | T | P | (position from user input) J-Ks=0.564+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:57:55.37 +72:12:02.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:57:55.37 +72:12:02.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.14 10:55:00.65 +68:11:49.4
137.84574 45.41231 galactic UMa Second-epoch detections are separated by 2.2" and 1.9 pix
The object was found in VSX 8" DDE 35
Type: UGZ+VY
# Max. Min./Amp. JD0 Period
14.700 r 19.900 r
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:55:00.65 +68:11:49.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:55:00.65 +68:11:49.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 10 55 00.65 +68 11 49.4 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
DDE 35,2461231.7332,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DDE 35 20260710.2332 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.93 13:13:18.60 +73:45:49.5
120.83476 43.27533 galactic UMi Second-epoch detections are separated by 1.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:18.60 +73:45:49.5 (user input) | T | P | (position from user input) J-Ks=0.690+/-0.035 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:18.60 +73:45:49.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:18.60 +73:45:49.5: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461231.7332,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.37 13:03:40.08 +72:56:33.9
121.68235 44.15582 galactic Dra Second-epoch detections are separated by 0.2" and 2.4 pix
The object was found in VSX 1" Gaia DR3 1688142500626030080
Type: ROT
# Max. Min./Amp. JD0 Period
13.020 G 13.080 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:03:40.08 +72:56:33.9: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:03:40.08 +72:56:33.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688142500626030080,2461231.7332,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688142500626030080 20260710.2332 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.01 13:14:12.33 +73:34:18.1
120.71733 43.45852 galactic UMi Second-epoch detections are separated by 2.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:12.33 +73:34:18.1 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:12.33 +73:34:18.1: 13.10 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:12.33 +73:34:18.1: 13.00 +/- 0.03 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,2461231.7332,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.35 13:15:36.50 +73:28:16.9
120.56392 43.54558 galactic UMi Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:36.50 +73:28:16.9 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.033 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:36.50 +73:28:16.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:36.50 +73:28:16.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.06 13:23:39.26 +71:27:43.0
119.29213 45.43794 galactic UMi Second-epoch detections are separated by 2.1" and 2.8 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 | 13:23:39.26 +71:27:43.0 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:23:39.26 +71:27:43.0: 13.06 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:23:39.26 +71:27:43.0: 13.03 +/- 0.03 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,2461231.7332,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.22 13:09:54.16 +73:23:10.0
121.10867 43.67671 galactic UMi Second-epoch detections are separated by 1.2" and 2.4 pix
The object was found in VSX 3" Gaia DR3 1688256025201698432
Type: ROT
# Max. Min./Amp. JD0 Period
12.660 G 12.680 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:09:54.16 +73:23:10.0: 13.07 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:09:54.16 +73:23:10.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688256025201698432,2461231.7332,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688256025201698432 20260710.2332 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.12 13:12:35.63 +73:33:51.5
120.87210 43.47923 galactic UMi Second-epoch detections are separated by 0.6" and 2.3 pix
The object was found in VSX 1" Gaia DR3 1688592475759640320
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:35.63 +73:33:51.5: 13.07 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:35.63 +73:33:51.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688592475759640320,2461231.7332,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688592475759640320 20260710.2332 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.10 13:19:32.20 +73:49:49.8
120.25623 43.15147 galactic UMi Second-epoch detections are separated by 0.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:32.20 +73:49:49.8 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.035 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:32.20 +73:49:49.8: 13.08 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:32.20 +73:49:49.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.54 10:40:28.72 +67:59:02.8
139.50313 44.69692 galactic UMa Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1072083558602613248 | 10:40:28.45 +67:59:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.121+/-0.030 (M)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:40:28.72 +67:59:02.8: 12.40 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:40:28.72 +67:59:02.8: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 10 40 28.72 +67 59 02.8 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
Gaia DR3 1072083558602613248,2461231.7332,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1072083558602613248 20260710.2332 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.88 13:13:41.14 +73:42:01.2
120.78862 43.33521 galactic UMi Second-epoch detections are separated by 0.8" and 2.4 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 | 13:13:41.14 +73:42:01.2 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.049 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:41.14 +73:42:01.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:41.14 +73:42:01.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461231.7332,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.87 13:14:52.81 +73:53:50.6
120.70798 43.12949 galactic UMi Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:52.81 +73:53:50.6 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.033 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:52.81 +73:53:50.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:52.81 +73:53:50.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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,2461231.7332,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.87 12:58:02.57 +72:22:51.4
122.22837 44.73828 galactic Dra Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:02.57 +72:22:51.4 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:02.57 +72:22:51.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:02.57 +72:22:51.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461231.7332,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.13 13:26:50.03 +71:29:44.7
118.94781 45.35769 galactic UMi Second-epoch detections are separated by 1.4" and 2.6 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 | 13:26:50.03 +71:29:44.7 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:26:50.03 +71:29:44.7: 13.04 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:26:50.03 +71:29:44.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.46 13:14:05.93 +73:07:24.3
120.65234 43.90439 galactic UMi Second-epoch detections are separated by 1.2" and 2.4 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 | Gaia DR3 1688201835598684416 | 13:14:05.95 +73:07:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.034 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:05.93 +73:07:24.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:05.93 +73:07:24.3: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688201835598684416,2461231.7332,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688201835598684416 20260710.2332 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.81 13:25:07.32 +71:30:29.2
119.14088 45.37138 galactic UMi Second-epoch detections are separated by 0.4" and 2.4 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 | 13:25:07.32 +71:30:29.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:25:07.32 +71:30:29.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:25:07.32 +71:30:29.2: 12.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.32 13:13:32.70 +72:42:16.8
120.63808 44.32499 galactic UMi Second-epoch detections are separated by 1.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:32.70 +72:42:16.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:32.70 +72:42:16.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:32.70 +72:42:16.8: 13.31 +/- 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,2461231.7332,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.11 13:04:18.19 +71:56:03.7
121.51806 45.15856 galactic UMi Second-epoch detections are separated by 1.7" and 2.6 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 | 13:04:18.19 +71:56:03.7 (user input) | T | P | (position from user input) J-Ks=0.560+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:04:18.19 +71:56:03.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:04:18.19 +71:56:03.7: 13.05 +/- 0.03 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,2461231.7332,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 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 07 10.2332 2461231.7332 12.06 10:36:39.39 +68:03:44.0
139.79413 44.39532 galactic UMa Second-epoch detections are separated by 2.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:36:39.39 +68:03:44.0 (user input) | T | P | (position from user input) J-Ks=0.700+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:39.39 +68:03:44.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:36:39.39 +68:03:44.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.2332* 10 36 39.39 +68 03 44.0 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,2461231.7332,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.08 12:52:14.30 +71:48:13.3
122.84304 45.32442 galactic Dra Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:52:14.30 +71:48:13.3 (user input) | T | P | (position from user input) J-Ks=0.286+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:52:14.30 +71:48:13.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:52:14.30 +71:48:13.3: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 12.12 13:01:03.03 +72:18:21.1
121.90275 44.80318 galactic Dra Second-epoch detections are separated by 1.2" and 2.4 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 | 13:01:03.03 +72:18:21.1 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.029 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:03.03 +72:18:21.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:03.03 +72:18:21.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.83 13:13:04.03 +72:55:31.3
120.72341 44.11002 galactic UMi Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:04.03 +72:55:31.3 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:04.03 +72:55:31.3: 13.02 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:04.03 +72:55:31.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.7332,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.2332 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.2332 2461231.7332 11.74 13:25:45.11 +69:57:02.1
118.64049 46.89071 galactic UMi Second-epoch detections are separated by 1.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1685357643831284224 | 13:25:45.08 +69:57:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:25:45.11 +69:57:02.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:25:45.11 +69:57:02.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1685357643831284224,2461231.7332,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1685357643831284224 20260710.2332 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461231.73343027 10.07.2026 05:35:58.375 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7377
Objects passed selection criteria: 7321
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 4561.75
Average stars matched: 4421.75 (96.931 %)
Memory usage VmPeak: 113272 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 00:54:00 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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461231.73343027 10.07.2026 05:35:58.375 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 109
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 39803
Objects passed selection criteria: 39683
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 25731.5
Average stars matched: 24759 (96.2206 %)
Memory usage VmPeak: 141748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 00:56:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461231.73293105
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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
Saving wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits to local_wcs_cache/
'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits exists and is non-empty
Saving wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits to local_wcs_cache/
'wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits'
wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.7'x627.1' 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: 11:59:37.960 +69:59:44.31 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-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Image size: 941.5'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 12:00:47.914 +69:58:56.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 12:00:47.914 +69:58:56.36
Angular distance between the image centers 0.1006 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Image size: 941.5'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 12:00:49.320 +69:59:06.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 12:00:49.320 +69:59:06.82
Angular distance between the image centers 0.1023 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 12:00:47.914 +69:58:56.36
Second-epoch second image center 12:00:49.320 +69:59:06.82
Angular distance between the image centers 0.00353 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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.tgd8rExtxk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits &> /tmp/tmp.48tYwT5xoL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits &> /tmp/tmp.Qy3aj83ub9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits &> /tmp/tmp.Hj7e7lRkkE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q1b1x1_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 151.6428 to 206.7164 deg, Dec +62.8285 to +75.5474 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 151.6428 to 206.7164 deg, Dec 62.8285 to 75.5474 deg
Loaded 8253 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): 4551 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 22.845900
a=0.000000 b=1.000000 c=22.845900
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 151.6428 to 206.7164 deg, Dec +62.8285 to +75.5474 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 151.6428 to 206.7164 deg, Dec 62.8285 to 75.5474 deg
Loaded 8253 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): 4551 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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=6.1)
Read 7626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6431 to 206.7164 deg, Dec +62.8284 to +75.5474 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 151.6431 to 206.7164 deg, Dec 62.8284 to 75.5474 deg
Loaded 8253 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): 4547 out of 4752 total matches.
Matched with Tycho-2 4752 out of 7626 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
2.7 pix fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
2.8 pix fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
2.1 pix wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Limiting magnitude estimates:
15.3 mag. Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.3 mag. Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
12.3 mag. fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
12.3 mag. fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
All-image limiting magnitude estimate: 12.3 (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.tgd8rExtxk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7645
Got 7645 stars (including 7087 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_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: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=960 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.345 n_q1=254 n_q2=230 n_q3=220 n_q4=256 worst_quadrant_to_overall_ratio=1.281
The image catalog is written to wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q1b1x1_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-Q1b1x1_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.48tYwT5xoL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=542, bad_region=0, passed=7626
Got 7626 stars (including 7073 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 7626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits N_match=960 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.303 n_q1=250 n_q2=234 n_q3=221 n_q4=255 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -region wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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.Qy3aj83ub9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=65, bad_region=0, passed=1548
Got 1548 stars (including 1482 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat
util/solve_plate_with_UCAC5 got 1548 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits N_match=954 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.316 n_q1=320 n_q2=280 n_q3=122 n_q4=232 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits -region wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.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.Hj7e7lRkkE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=58, bad_region=0, passed=1525
Got 1525 stars (including 1466 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat
util/solve_plate_with_UCAC5 got 1525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 1495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 1493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 1493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits N_match=952 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.280 n_q1=275 n_q2=291 n_q3=131 n_q4=255 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits -region wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits sigma_overall=0.375 worst_q_ratio=1.281
ref2=Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits sigma_overall=0.357 worst_q_ratio=1.316
new1=fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits sigma_overall=0.346 worst_q_ratio=1.141
new2=fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits sigma_overall=0.313 worst_q_ratio=1.272
reference average sigma_overall=0.366 worst_q_ratio=1.2985
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294_astrometric_residuals.png (960 matched stars from wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295_astrometric_residuals.png (960 matched stars from wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168_astrometric_residuals.png (954 matched stars from wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169_astrometric_residuals.png (952 matched stars from wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.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-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits'
Preparing the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.7'x627.1' 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: 11:59:37.960 +69:59:44.31 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-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Image size: 941.5'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 12:00:47.914 +69:58:56.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 12:00:47.914 +69:58:56.36
Angular distance between the image centers 0.1006 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Image size: 941.5'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 12:00:49.320 +69:59:06.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 12:00:49.320 +69:59:06.82
Angular distance between the image centers 0.1023 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 12:00:47.914 +69:58:56.36
Second-epoch second image center 12:00:49.320 +69:59:06.82
Angular distance between the image centers 0.00353 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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.1jzPo0zgkn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits &> /tmp/tmp.yQelgJWNH9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits &> /tmp/tmp.RLeRbbc38v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits &> /tmp/tmp.tiSM6SlldH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q1b1x1_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 151.3664 to 206.9040 deg, Dec +62.7303 to +75.5592 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 151.3664 to 206.9040 deg, Dec 62.7303 to 75.5592 deg
Loaded 8396 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): 4348 out of 4842 total matches.
Matched with Tycho-2 4842 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 22.746950
a=0.000000 b=1.000000 c=22.746950
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
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 151.3664 to 206.9040 deg, Dec +62.7303 to +75.5592 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 151.3664 to 206.9040 deg, Dec 62.7303 to 75.5592 deg
Loaded 8396 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): 4348 out of 4842 total matches.
Matched with Tycho-2 4842 out of 42210 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=4.9)
Read 42071 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3666 to 206.9042 deg, Dec +62.7305 to +75.5474 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 151.3666 to 206.9042 deg, Dec 62.7305 to 75.5474 deg
Loaded 8393 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): 4349 out of 4835 total matches.
Matched with Tycho-2 4835 out of 42071 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 99 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.0 pix Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
2.6 pix fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
2.6 pix fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
2.0 pix wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.0 pix wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Limiting magnitude estimates:
15.4 mag. Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.4 mag. Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
12.8 mag. fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
12.8 mag. fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.5 (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.1jzPo0zgkn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2006, bad_region=4, passed=42192
Got 42192 stars (including 40113 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 42192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 41589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 41586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 41586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=966 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.346 n_q1=256 n_q2=235 n_q3=223 n_q4=252 worst_quadrant_to_overall_ratio=1.240
The image catalog is written to wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q1b1x1_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-Q1b1x1_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.yQelgJWNH9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1960, bad_region=8, passed=42051
Got 42051 stars (including 40002 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 42051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 41432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 41435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 41435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits N_match=964 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.306 n_q1=256 n_q2=233 n_q3=224 n_q4=251 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -region wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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.RLeRbbc38v (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=178, bad_region=2, passed=9810
Got 9810 stars (including 9607 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat
util/solve_plate_with_UCAC5 got 9810 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 9438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 9438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits N_match=950 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.306 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.332 n_q1=321 n_q2=280 n_q3=122 n_q4=227 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits -region wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.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.tiSM6SlldH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=149, bad_region=2, passed=9542
Got 9542 stars (including 9378 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat
util/solve_plate_with_UCAC5 got 9542 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 9295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 9296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 9296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits N_match=946 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.274 n_q1=275 n_q2=289 n_q3=129 n_q4=253 worst_quadrant_to_overall_ratio=1.263
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits -region wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.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-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-15_20.00sec_-0.00C_LIGHTs_0168.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Dra-03-Q1b1x1_004759_TTUQ1b1x1_1720788_aiSt9Xdo/wcs_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169.fits
Preparing the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:05:35.68 +65:32:54.4: 12.42 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:05:35.68 +65:32:54.4: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 11:05:35.68 +65:32:54.4: ref_mag=12.42 +/- 0.01 new_mean_mag=12.1017 delta=0.32 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:26:41.19 +69:58:38.4: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:38.77 +73:42:31.5: 13.75 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:01.29 +68:57:59.3: 13.06 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:03:29.52 +72:40:30.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:50.82 +72:20:36.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:09.51 +72:58:11.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:27:03.14 +69:12:18.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:34.04 +73:17:51.8: 13.62 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:26:41.19 +69:58:38.4: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:50.82 +72:20:36.1: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:03:29.52 +72:40:30.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 13:01:50.82 +72:20:36.1: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9790 delta=0.91 (need > 0.90)
Forced photometry filter KEPT candidate at 13:26:41.19 +69:58:38.4: ref_mag=12.80 +/- 0.02 new_mean_mag=11.8921 delta=0.90 (need > 0.90)
Forced photometry filter KEPT candidate at 13:03:29.52 +72:40:30.8: ref_mag=13.44 +/- 0.03 new_mean_mag=12.4618 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:09.51 +72:58:11.6: 13.78 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:38.77 +73:42:31.5: 13.87 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:34:01.29 +68:57:59.3: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:27:03.14 +69:12:18.1: 12.64 +/- 0.02 detection
Forced photometry filter KEPT candidate at 13:15:38.77 +73:42:31.5: ref_mag=13.81 +/- 0.04 new_mean_mag=12.6184 delta=1.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 10:34:01.29 +68:57:59.3: ref_mag=13.04 +/- 0.02 new_mean_mag=12.1032 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 13:11:09.51 +72:58:11.6: ref_mag=13.73 +/- 0.03 new_mean_mag=12.4605 delta=1.26 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 13:27:03.14 +69:12:18.1: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6540 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:34.04 +73:17:51.8: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 13:19:34.04 +73:17:51.8: ref_mag=13.55 +/- 0.03 new_mean_mag=12.4826 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:09:38.14 +72:43:43.4: 13.60 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:09.40 +72:57:01.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:09:38.14 +72:43:43.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 13:09:38.14 +72:43:43.4: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5691 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:09.40 +72:57:01.0: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 13:13:09.40 +72:57:01.0: ref_mag=13.39 +/- 0.03 new_mean_mag=12.2596 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:46.07 +72:34:36.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:46.07 +72:34:36.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 13:11:46.07 +72:34:36.4: ref_mag=13.43 +/- 0.03 new_mean_mag=12.2181 delta=1.21 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:11.71 +73:25:37.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:10:15.05 +68:32:04.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:11.71 +73:25:37.5: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter KEPT candidate at 13:19:11.71 +73:25:37.5: ref_mag=13.37 +/- 0.03 new_mean_mag=12.2773 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:10:15.05 +68:32:04.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.01
Forced photometry filter KEPT candidate at 11:10:15.05 +68:32:04.6: ref_mag=12.98 +/- 0.01 new_mean_mag=12.0360 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:33:45.63 +72:36:21.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:33:45.63 +72:36:21.5: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 13:33:45.63 +72:36:21.5: ref_mag=13.21 +/- 0.02 new_mean_mag=12.1967 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:39.19 +67:34:15.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:56:45.03 +72:15:19.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:41:39.19 +67:34:15.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 10:41:39.19 +67:34:15.8: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0479 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:09.60 +72:48:42.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:56:45.03 +72:15:19.7: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 12:56:45.03 +72:15:19.7: ref_mag=12.58 +/- 0.01 new_mean_mag=11.6631 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:55.43 +72:54:06.5: 12.56 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:09.60 +72:48:42.3: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 13:11:09.60 +72:48:42.3: ref_mag=13.40 +/- 0.03 new_mean_mag=12.3547 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:46.85 +73:20:22.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:55.43 +72:54:06.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 13:13:55.43 +72:54:06.5: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6078 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:46.85 +73:20:22.3: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:46.85 +73:20:22.3: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1974 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:55.52 +73:00:02.8: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:10:14.06 +73:53:08.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:55.52 +73:00:02.8: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:55.52 +73:00:02.8: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1175 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:10:14.06 +73:53:08.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 13:10:14.06 +73:53:08.4: ref_mag=13.51 +/- 0.03 new_mean_mag=12.4567 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:11:30.58 +72:57:37.3: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:11:30.58 +72:57:37.3: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 13:11:30.58 +72:57:37.3: ref_mag=13.54 +/- 0.03 new_mean_mag=12.4213 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:35.16 +72:59:47.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:35.16 +72:59:47.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 13:12:35.16 +72:59:47.9: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9156 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:21:06.13 +73:48:02.9: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:21:06.13 +73:48:02.9: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 13:21:06.13 +73:48:02.9: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9442 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:01.20 +72:35:11.1: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:01.20 +72:35:11.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 13:01:01.20 +72:35:11.1: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9532 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:13.84 +72:38:48.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:13.84 +72:38:48.1: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 12:58:13.84 +72:38:48.1: ref_mag=13.54 +/- 0.03 new_mean_mag=12.5246 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:20:11.43 +73:26:09.2: 12.93 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:02:07.69 +71:56:19.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:20:11.43 +73:26:09.2: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 13:20:11.43 +73:26:09.2: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9201 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:02:07.69 +71:56:19.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 13:02:07.69 +71:56:19.7: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9780 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:38:16.62 +68:02:21.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:43.56 +73:10:10.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:38:16.62 +68:02:21.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 10:38:16.62 +68:02:21.6: ref_mag=12.90 +/- 0.02 new_mean_mag=11.9772 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:43.56 +73:10:10.7: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:43.56 +73:10:10.7: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0507 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:16.71 +68:14:23.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:18.51 +73:18:18.9: 13.35 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:36:16.71 +68:14:23.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 10:36:16.71 +68:14:23.5: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1315 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:18.51 +73:18:18.9: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 13:13:18.51 +73:18:18.9: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4089 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:08.49 +72:32:32.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:08.49 +72:32:32.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:08.49 +72:32:32.2: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1624 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:27.75 +73:56:33.9: 13.76 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:27.75 +73:56:33.9: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 13:14:27.75 +73:56:33.9: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5464 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:00.24 +73:47:23.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:00.24 +73:47:23.9: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 13:15:00.24 +73:47:23.9: ref_mag=13.58 +/- 0.03 new_mean_mag=12.4771 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:23:25.77 +71:20:57.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:23:25.77 +71:20:57.4: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 13:23:25.77 +71:20:57.4: ref_mag=12.94 +/- 0.02 new_mean_mag=12.0146 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:03.43 +72:40:46.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:03.43 +72:40:46.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 12:58:03.43 +72:40:46.9: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9553 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:26.52 +72:59:51.6: 13.71 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:16:23.22 +73:16:26.1: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:26.52 +72:59:51.6: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 13:12:26.52 +72:59:51.6: ref_mag=13.71 +/- 0.03 new_mean_mag=12.5355 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:07.81 +73:49:12.6: 12.91 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:16:23.22 +73:16:26.1: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 13:16:23.22 +73:16:26.1: ref_mag=13.58 +/- 0.03 new_mean_mag=12.4309 delta=1.15 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:07.81 +73:49:12.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:07.81 +73:49:12.6: ref_mag=12.91 +/- 0.02 new_mean_mag=11.9867 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:32.95 +72:41:52.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:39.99 +73:30:53.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:32.95 +72:41:52.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:32.95 +72:41:52.7: ref_mag=12.88 +/- 0.02 new_mean_mag=11.9281 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:39.99 +73:30:53.6: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 13:15:39.99 +73:30:53.6: ref_mag=13.56 +/- 0.03 new_mean_mag=12.5035 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:22:47.96 +73:44:58.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:22:47.96 +73:44:58.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 13:22:47.96 +73:44:58.3: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1697 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:40:26.28 +67:31:06.6: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:18:25.42 +73:11:59.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:40:26.28 +67:31:06.6: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 10:40:26.28 +67:31:06.6: ref_mag=12.87 +/- 0.02 new_mean_mag=11.8623 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:18:25.42 +73:11:59.8: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 13:18:25.42 +73:11:59.8: ref_mag=12.85 +/- 0.02 new_mean_mag=11.9353 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:22:31.96 +73:39:29.4: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:22:31.96 +73:39:29.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter KEPT candidate at 13:22:31.96 +73:39:29.4: ref_mag=12.79 +/- 0.02 new_mean_mag=11.8708 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:19.78 +72:16:20.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:19.78 +72:16:20.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 12:58:19.78 +72:16:20.8: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8790 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:57:55.37 +72:12:02.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:55:00.65 +68:11:49.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:57:55.37 +72:12:02.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 12:57:55.37 +72:12:02.2: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2367 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:55:00.65 +68:11:49.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 10:55:00.65 +68:11:49.4: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1510 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:18.60 +73:45:49.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:18.60 +73:45:49.5: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:18.60 +73:45:49.5: ref_mag=12.84 +/- 0.02 new_mean_mag=11.9186 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:03:40.08 +72:56:33.9: 13.32 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:03:40.08 +72:56:33.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 13:03:40.08 +72:56:33.9: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2913 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:12.33 +73:34:18.1: 13.10 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:15:36.50 +73:28:16.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:12.33 +73:34:18.1: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:12.33 +73:34:18.1: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0048 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:15:36.50 +73:28:16.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 13:15:36.50 +73:28:16.9: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3586 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:23:39.26 +71:27:43.0: 13.06 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:23:39.26 +71:27:43.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 13:23:39.26 +71:27:43.0: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0843 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:09:54.16 +73:23:10.0: 13.07 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:09:54.16 +73:23:10.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 13:09:54.16 +73:23:10.0: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1471 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:12:35.63 +73:33:51.5: 13.07 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:12:35.63 +73:33:51.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 13:12:35.63 +73:33:51.5: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1280 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:19:32.20 +73:49:49.8: 13.08 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:19:32.20 +73:49:49.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 13:19:32.20 +73:49:49.8: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0731 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:40:28.72 +67:59:02.8: 12.40 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:41.14 +73:42:01.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:40:28.72 +67:59:02.8: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 10:40:28.72 +67:59:02.8: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4474 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:41.14 +73:42:01.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:41.14 +73:42:01.2: ref_mag=12.80 +/- 0.02 new_mean_mag=11.8703 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:52.81 +73:53:50.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:52.81 +73:53:50.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter KEPT candidate at 13:14:52.81 +73:53:50.6: ref_mag=12.79 +/- 0.02 new_mean_mag=11.8707 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:58:02.57 +72:22:51.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:58:02.57 +72:22:51.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 12:58:02.57 +72:22:51.4: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8574 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:26:50.03 +71:29:44.7: 13.04 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:26:50.03 +71:29:44.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 13:26:50.03 +71:29:44.7: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1332 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:14:05.93 +73:07:24.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:14:05.93 +73:07:24.3: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 13:14:05.93 +73:07:24.3: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4578 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:25:07.32 +71:30:29.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:38:55.18 +68:29:54.5: 12.46 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:25:07.32 +71:30:29.2: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter KEPT candidate at 13:25:07.32 +71:30:29.2: ref_mag=12.75 +/- 0.01 new_mean_mag=11.8188 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:38:55.18 +68:29:54.5: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 10:38:55.18 +68:29:54.5: ref_mag=12.49 +/- 0.01 new_mean_mag=11.7869 delta=0.70 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:32.70 +72:42:16.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:04:18.19 +71:56:03.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:32.70 +72:42:16.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:32.70 +72:42:16.8: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2610 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:04:18.19 +71:56:03.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 13:04:18.19 +71:56:03.7: ref_mag=13.04 +/- 0.02 new_mean_mag=12.1162 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:39.39 +68:03:44.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 10:36:39.39 +68:03:44.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 10:36:39.39 +68:03:44.0: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0463 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:52:14.30 +71:48:13.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:01:03.03 +72:18:21.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:52:14.30 +71:48:13.3: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 12:52:14.30 +71:48:13.3: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0344 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:01:03.03 +72:18:21.1: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 13:01:03.03 +72:18:21.1: ref_mag=13.03 +/- 0.02 new_mean_mag=12.1155 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:13:04.03 +72:55:31.3: 13.02 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:13:04.03 +72:55:31.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 13:13:04.03 +72:55:31.3: ref_mag=12.96 +/- 0.02 new_mean_mag=11.8239 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 13:25:45.11 +69:57:02.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 13:25:45.11 +69:57:02.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 13:25:45.11 +69:57:02.1: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6893 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out16975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41820.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 101s
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: 34s
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Considering the candidate 52809_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52809_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
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Considering the candidate 52864_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52864_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 52882_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52882_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 52886_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52886_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 52892_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52892_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 52909_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52909_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 52932_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52932_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 52948_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 52948_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 53078_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53078_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 53131_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53131_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 53155_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53155_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 53349_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53349_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 53380_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53380_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 53381_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53381_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 12:05:58.33 +68:46:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53429_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53429_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 53436_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53436_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 53672_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53672_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 12:57:05.74 +71:26:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53673_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53673_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 53719_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 53719_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 20102_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 20102_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41757_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41757_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 39721_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 39721_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 34402_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34402_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 38259_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38259_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37312_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37312_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 35859_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 35859_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 16975_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 16975_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 23927_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 23927_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 11:19:05.07 +70:06:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38041_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38041_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37311_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37311_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 38678_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38678_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 35359_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 35359_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 18857_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 18857_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29378_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29378_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 19791_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 19791_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29958_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29958_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29524_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29524_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29374_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29374_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29205_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29205_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37067_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37067_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33936_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33936_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37143_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37143_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37199_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37199_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33868_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33868_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29694_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29694_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 38860_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38860_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29154_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29154_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29995_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29995_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 22182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 22182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 36367_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 36367_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 23296_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 23296_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29240_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29240_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 38725_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38725_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33628_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33628_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 28998_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 28998_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 30367_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 30367_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29643_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29643_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 36930_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 36930_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 36012_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 36012_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 34129_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34129_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 38080_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 38080_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 35186_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 35186_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33946_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33946_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 19830_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 19830_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 36182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 36182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 23249_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 23249_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 10:44:38.71 +68:46:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34142_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34142_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 39843_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 39843_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 40318_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 40318_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 19814_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 19814_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 34353_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34353_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29457_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29457_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 34913_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34913_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 35374_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 35374_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41820_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41820_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 35796_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 35796_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 29083_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29083_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33788_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33788_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 21502_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 21502_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 34661_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 34661_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 33873_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 33873_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 39767_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 39767_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41521_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41521_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 36507_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 36507_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41679_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41679_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 23786_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 23786_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
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Considering the candidate 35430_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 35430_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 10:55:41.54 +71:52:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29602_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 29602_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41182_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 22612_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 22612_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 41662_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 41662_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 39952_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 39952_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 37359_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 37359_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 19896_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
Preparing report for the candidate 19896_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
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Considering the candidate 18099_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 18099_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 11:31:24.45 +69:19:53.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 14729_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 14729_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 12:30:06.09 +69:12:04.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17232_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 17232_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 12:33:28.00 +69:47:21.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 08154_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 08154_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 11:42:28.24 +66:44:44.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18048_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169
The candidate 18048_fd_Dra-03-Q1b1x1_2026-07-10_00-35-58_20.00sec_-0.00C_LIGHTs_0169 did not pass the final checks
**** FOUND 10:45:04.30 +67:24:42.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 140s
Prepared the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:27:03.14 +69:12:18.1
11:10:15.05 +68:32:04.6
10:41:39.19 +67:34:15.8
10:55:00.65 +68:11:49.4
10:40:26.28 +67:31:06.6
13:25:45.11 +69:57:02.1
13:26:41.19 +69:58:38.4
10:40:28.72 +67:59:02.8
10:38:16.62 +68:02:21.6
10:36:39.39 +68:03:44.0
10:36:16.71 +68:14:23.5
13:15:00.24 +73:47:23.9
13:12:35.63 +73:33:51.5
13:20:11.43 +73:26:09.2
13:19:46.85 +73:20:22.3
13:13:18.51 +73:18:18.9
13:13:55.43 +72:54:06.5
13:33:45.63 +72:36:21.5
13:03:40.08 +72:56:33.9
13:11:09.60 +72:48:42.3
13:13:32.70 +72:42:16.8
12:58:03.43 +72:40:46.9
13:01:01.20 +72:35:11.1
12:56:45.03 +72:15:19.7
13:02:07.69 +71:56:19.7
13:23:25.77 +71:20:57.4
13:14:27.75 +73:56:33.9
13:19:32.20 +73:49:49.8
13:21:06.13 +73:48:02.9
13:14:52.81 +73:53:50.6
13:10:14.06 +73:53:08.4
13:22:47.96 +73:44:58.3
13:13:07.81 +73:49:12.6
13:22:31.96 +73:39:29.4
13:13:18.60 +73:45:49.5
13:15:38.77 +73:42:31.5
13:13:41.14 +73:42:01.2
13:14:12.33 +73:34:18.1
13:15:39.99 +73:30:53.6
13:19:11.71 +73:25:37.5
13:15:36.50 +73:28:16.9
13:09:54.16 +73:23:10.0
13:19:34.04 +73:17:51.8
13:16:23.22 +73:16:26.1
13:18:25.42 +73:11:59.8
13:15:43.56 +73:10:10.7
13:14:05.93 +73:07:24.3
13:12:26.52 +72:59:51.6
13:15:55.52 +73:00:02.8
13:11:30.58 +72:57:37.3
13:12:35.16 +72:59:47.9
13:13:09.40 +72:57:01.0
13:11:09.51 +72:58:11.6
13:13:04.03 +72:55:31.3
13:09:38.14 +72:43:43.4
13:14:32.95 +72:41:52.7
13:03:29.52 +72:40:30.8
13:11:46.07 +72:34:36.4
13:14:08.49 +72:32:32.2
12:58:13.84 +72:38:48.1
13:01:50.82 +72:20:36.1
12:58:02.57 +72:22:51.4
12:58:19.78 +72:16:20.8
13:01:03.03 +72:18:21.1
12:57:55.37 +72:12:02.2
13:04:18.19 +71:56:03.7
13:26:50.03 +71:29:44.7
12:52:14.30 +71:48:13.3
13:25:07.32 +71:30:29.2
10:34:01.29 +68:57:59.3
13:23:39.26 +71:27:43.0
########### Completed Dra-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
13:26:41.19 +69:58:38.4
10:34:01.29 +68:57:59.3
13:01:50.82 +72:20:36.1
13:15:38.77 +73:42:31.5
13:03:29.52 +72:40:30.8
13:11:09.51 +72:58:11.6
13:19:34.04 +73:17:51.8
13:27:03.14 +69:12:18.1
13:09:38.14 +72:43:43.4
13:13:09.40 +72:57:01.0
13:11:46.07 +72:34:36.4
13:19:11.71 +73:25:37.5
11:10:15.05 +68:32:04.6
13:33:45.63 +72:36:21.5
10:41:39.19 +67:34:15.8
12:56:45.03 +72:15:19.7
13:11:09.60 +72:48:42.3
13:13:55.43 +72:54:06.5
13:19:46.85 +73:20:22.3
13:15:55.52 +73:00:02.8
13:10:14.06 +73:53:08.4
13:11:30.58 +72:57:37.3
13:12:35.16 +72:59:47.9
13:21:06.13 +73:48:02.9
13:01:01.20 +72:35:11.1
12:58:13.84 +72:38:48.1
13:20:11.43 +73:26:09.2
13:02:07.69 +71:56:19.7
10:38:16.62 +68:02:21.6
13:15:43.56 +73:10:10.7
10:36:16.71 +68:14:23.5
13:13:18.51 +73:18:18.9
13:14:08.49 +72:32:32.2
13:14:27.75 +73:56:33.9
13:15:00.24 +73:47:23.9
13:23:25.77 +71:20:57.4
12:58:03.43 +72:40:46.9
13:12:26.52 +72:59:51.6
13:16:23.22 +73:16:26.1
13:13:07.81 +73:49:12.6
13:14:32.95 +72:41:52.7
13:15:39.99 +73:30:53.6
13:22:47.96 +73:44:58.3
10:40:26.28 +67:31:06.6
13:18:25.42 +73:11:59.8
13:22:31.96 +73:39:29.4
12:58:19.78 +72:16:20.8
12:57:55.37 +72:12:02.2
10:55:00.65 +68:11:49.4
13:13:18.60 +73:45:49.5
13:03:40.08 +72:56:33.9
13:14:12.33 +73:34:18.1
13:15:36.50 +73:28:16.9
13:23:39.26 +71:27:43.0
13:09:54.16 +73:23:10.0
13:12:35.63 +73:33:51.5
13:19:32.20 +73:49:49.8
10:40:28.72 +67:59:02.8
13:13:41.14 +73:42:01.2
13:14:52.81 +73:53:50.6
12:58:02.57 +72:22:51.4
13:26:50.03 +71:29:44.7
13:14:05.93 +73:07:24.3
13:25:07.32 +71:30:29.2
13:13:32.70 +72:42:16.8
13:04:18.19 +71:56:03.7
10:36:39.39 +68:03:44.0
12:52:14.30 +71:48:13.3
13:01:03.03 +72:18:21.1
13:13:04.03 +72:55:31.3
13:25:45.11 +69:57:02.1
###################################################################################
13:26:41.19 +69:58:38.4 -- not an asteroid (will add it to exclusion list)
10:34:01.29 +68:57:59.3 -- not an asteroid (will add it to exclusion list)
13:01:50.82 +72:20:36.1 -- not an asteroid (will add it to exclusion list)
13:15:38.77 +73:42:31.5 -- not an asteroid (will add it to exclusion list)
13:03:29.52 +72:40:30.8 -- not an asteroid (will add it to exclusion list)
13:11:09.51 +72:58:11.6 -- not an asteroid (will add it to exclusion list)
13:19:34.04 +73:17:51.8 -- not an asteroid (will add it to exclusion list)
13:27:03.14 +69:12:18.1 -- not an asteroid (will add it to exclusion list)
13:09:38.14 +72:43:43.4 -- not an asteroid (will add it to exclusion list)
13:13:09.40 +72:57:01.0 -- not an asteroid (will add it to exclusion list)
13:11:46.07 +72:34:36.4 -- not an asteroid (will add it to exclusion list)
13:19:11.71 +73:25:37.5 -- not an asteroid (will add it to exclusion list)
11:10:15.05 +68:32:04.6 -- not an asteroid (will add it to exclusion list)
13:33:45.63 +72:36:21.5 -- not an asteroid (will add it to exclusion list)
10:41:39.19 +67:34:15.8 -- not an asteroid (will add it to exclusion list)
12:56:45.03 +72:15:19.7 -- not an asteroid (will add it to exclusion list)
13:11:09.60 +72:48:42.3 -- not an asteroid (will add it to exclusion list)
13:13:55.43 +72:54:06.5 -- not an asteroid (will add it to exclusion list)
13:19:46.85 +73:20:22.3 -- not an asteroid (will add it to exclusion list)
13:15:55.52 +73:00:02.8 -- not an asteroid (will add it to exclusion list)
13:10:14.06 +73:53:08.4 -- not an asteroid (will add it to exclusion list)
13:11:30.58 +72:57:37.3 -- not an asteroid (will add it to exclusion list)
13:12:35.16 +72:59:47.9 -- not an asteroid (will add it to exclusion list)
13:21:06.13 +73:48:02.9 -- not an asteroid (will add it to exclusion list)
13:01:01.20 +72:35:11.1 -- not an asteroid (will add it to exclusion list)
12:58:13.84 +72:38:48.1 -- not an asteroid (will add it to exclusion list)
13:20:11.43 +73:26:09.2 -- not an asteroid (will add it to exclusion list)
13:02:07.69 +71:56:19.7 -- not an asteroid (will add it to exclusion list)
10:38:16.62 +68:02:21.6 -- not an asteroid (will add it to exclusion list)
13:15:43.56 +73:10:10.7 -- not an asteroid (will add it to exclusion list)
10:36:16.71 +68:14:23.5 -- not an asteroid (will add it to exclusion list)
13:13:18.51 +73:18:18.9 -- not an asteroid (will add it to exclusion list)
13:14:08.49 +72:32:32.2 -- not an asteroid (will add it to exclusion list)
13:14:27.75 +73:56:33.9 -- not an asteroid (will add it to exclusion list)
13:15:00.24 +73:47:23.9 -- not an asteroid (will add it to exclusion list)
13:23:25.77 +71:20:57.4 -- not an asteroid (will add it to exclusion list)
12:58:03.43 +72:40:46.9 -- not an asteroid (will add it to exclusion list)
13:12:26.52 +72:59:51.6 -- not an asteroid (will add it to exclusion list)
13:16:23.22 +73:16:26.1 -- not an asteroid (will add it to exclusion list)
13:13:07.81 +73:49:12.6 -- not an asteroid (will add it to exclusion list)
13:14:32.95 +72:41:52.7 -- not an asteroid (will add it to exclusion list)
13:15:39.99 +73:30:53.6 -- not an asteroid (will add it to exclusion list)
13:22:47.96 +73:44:58.3 -- not an asteroid (will add it to exclusion list)
10:40:26.28 +67:31:06.6 -- not an asteroid (will add it to exclusion list)
13:18:25.42 +73:11:59.8 -- not an asteroid (will add it to exclusion list)
13:22:31.96 +73:39:29.4 -- not an asteroid (will add it to exclusion list)
12:58:19.78 +72:16:20.8 -- not an asteroid (will add it to exclusion list)
12:57:55.37 +72:12:02.2 -- not an asteroid (will add it to exclusion list)
10:55:00.65 +68:11:49.4 -- not an asteroid (will add it to exclusion list)
13:13:18.60 +73:45:49.5 -- not an asteroid (will add it to exclusion list)
13:03:40.08 +72:56:33.9 -- not an asteroid (will add it to exclusion list)
13:14:12.33 +73:34:18.1 -- not an asteroid (will add it to exclusion list)
13:15:36.50 +73:28:16.9 -- not an asteroid (will add it to exclusion list)
13:23:39.26 +71:27:43.0 -- not an asteroid (will add it to exclusion list)
13:09:54.16 +73:23:10.0 -- not an asteroid (will add it to exclusion list)
13:12:35.63 +73:33:51.5 -- not an asteroid (will add it to exclusion list)
13:19:32.20 +73:49:49.8 -- not an asteroid (will add it to exclusion list)
10:40:28.72 +67:59:02.8 -- not an asteroid (will add it to exclusion list)
13:13:41.14 +73:42:01.2 -- not an asteroid (will add it to exclusion list)
13:14:52.81 +73:53:50.6 -- not an asteroid (will add it to exclusion list)
12:58:02.57 +72:22:51.4 -- not an asteroid (will add it to exclusion list)
13:26:50.03 +71:29:44.7 -- not an asteroid (will add it to exclusion list)
13:14:05.93 +73:07:24.3 -- not an asteroid (will add it to exclusion list)
13:25:07.32 +71:30:29.2 -- not an asteroid (will add it to exclusion list)
13:13:32.70 +72:42:16.8 -- not an asteroid (will add it to exclusion list)
13:04:18.19 +71:56:03.7 -- not an asteroid (will add it to exclusion list)
10:36:39.39 +68:03:44.0 -- not an asteroid (will add it to exclusion list)
12:52:14.30 +71:48:13.3 -- not an asteroid (will add it to exclusion list)
13:01:03.03 +72:18:21.1 -- not an asteroid (will add it to exclusion list)
13:13:04.03 +72:55:31.3 -- not an asteroid (will add it to exclusion list)
13:25:45.11 +69:57:02.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:34:01.29 +68:57:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:16.71 +68:14:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:39.39 +68:03:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:38:16.62 +68:02:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:40:26.28 +67:31:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:40:28.72 +67:59:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:39.19 +67:34:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:55:00.65 +68:11:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:10:15.05 +68:32:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:14.30 +71:48:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:45.03 +72:15:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:55.37 +72:12:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:02.57 +72:22:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:03.43 +72:40:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:13.84 +72:38:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:19.78 +72:16:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:01.20 +72:35:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:03.03 +72:18:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:50.82 +72:20:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:07.69 +71:56:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:29.52 +72:40:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:40.08 +72:56:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:18.19 +71:56:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:38.14 +72:43:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:54.16 +73:23:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:14.06 +73:53:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:09.51 +72:58:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:09.60 +72:48:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:30.58 +72:57:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:46.07 +72:34:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:26.52 +72:59:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:35.16 +72:59:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:35.63 +73:33:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:04.03 +72:55:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:07.81 +73:49:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:09.40 +72:57:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:18.51 +73:18:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:18.60 +73:45:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:32.70 +72:42:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:41.14 +73:42:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:55.43 +72:54:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:05.93 +73:07:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:08.49 +72:32:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:12.33 +73:34:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:27.75 +73:56:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:32.95 +72:41:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:52.81 +73:53:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:00.24 +73:47:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:36.50 +73:28:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:38.77 +73:42:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:39.99 +73:30:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:43.56 +73:10:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:55.52 +73:00:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:23.22 +73:16:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:25.42 +73:11:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:11.71 +73:25:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:32.20 +73:49:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:34.04 +73:17:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:46.85 +73:20:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:11.43 +73:26:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:06.13 +73:48:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:31.96 +73:39:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:47.96 +73:44:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:25.77 +71:20:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:39.26 +71:27:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:07.32 +71:30:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:45.11 +69:57:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:41.19 +69:58:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:50.03 +71:29:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:03.14 +69:12:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:45.63 +72:36:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:34:01.29 +68:57:59.3 -- not a known variable star
10:36:16.71 +68:14:23.5 -- not a known variable star
10:36:39.39 +68:03:44.0 -- not a known variable star
10:38:16.62 +68:02:21.6 -- not a known variable star
10:40:26.28 +67:31:06.6 -- not a known variable star
10:40:28.72 +67:59:02.8 -- not a known variable star
10:41:39.19 +67:34:15.8 -- not a known variable star
10:55:00.65 +68:11:49.4 -- a known variable star
11:10:15.05 +68:32:04.6 -- not a known variable star
12:52:14.30 +71:48:13.3 -- not a known variable star
12:56:45.03 +72:15:19.7 -- not a known variable star
12:57:55.37 +72:12:02.2 -- not a known variable star
12:58:02.57 +72:22:51.4 -- not a known variable star
12:58:03.43 +72:40:46.9 -- not a known variable star
12:58:13.84 +72:38:48.1 -- not a known variable star
12:58:19.78 +72:16:20.8 -- not a known variable star
13:01:01.20 +72:35:11.1 -- a known variable star
13:01:03.03 +72:18:21.1 -- not a known variable star
13:01:50.82 +72:20:36.1 -- not a known variable star
13:02:07.69 +71:56:19.7 -- not a known variable star
13:03:29.52 +72:40:30.8 -- not a known variable star
13:03:40.08 +72:56:33.9 -- a known variable star
13:04:18.19 +71:56:03.7 -- not a known variable star
13:09:38.14 +72:43:43.4 -- not a known variable star
13:09:54.16 +73:23:10.0 -- a known variable star
13:10:14.06 +73:53:08.4 -- not a known variable star
13:11:09.51 +72:58:11.6 -- not a known variable star
13:11:09.60 +72:48:42.3 -- not a known variable star
13:11:30.58 +72:57:37.3 -- not a known variable star
13:11:46.07 +72:34:36.4 -- not a known variable star
13:12:26.52 +72:59:51.6 -- not a known variable star
13:12:35.16 +72:59:47.9 -- not a known variable star
13:12:35.63 +73:33:51.5 -- a known variable star
13:13:04.03 +72:55:31.3 -- not a known variable star
13:13:07.81 +73:49:12.6 -- not a known variable star
13:13:09.40 +72:57:01.0 -- a known variable star
13:13:18.51 +73:18:18.9 -- not a known variable star
13:13:18.60 +73:45:49.5 -- not a known variable star
13:13:32.70 +72:42:16.8 -- not a known variable star
13:13:41.14 +73:42:01.2 -- not a known variable star
13:13:55.43 +72:54:06.5 -- not a known variable star
13:14:05.93 +73:07:24.3 -- not a known variable star
13:14:08.49 +72:32:32.2 -- not a known variable star
13:14:12.33 +73:34:18.1 -- not a known variable star
13:14:27.75 +73:56:33.9 -- not a known variable star
13:14:32.95 +72:41:52.7 -- not a known variable star
13:14:52.81 +73:53:50.6 -- not a known variable star
13:15:00.24 +73:47:23.9 -- not a known variable star
13:15:36.50 +73:28:16.9 -- not a known variable star
13:15:38.77 +73:42:31.5 -- not a known variable star
13:15:39.99 +73:30:53.6 -- not a known variable star
13:15:43.56 +73:10:10.7 -- not a known variable star
13:15:55.52 +73:00:02.8 -- not a known variable star
13:16:23.22 +73:16:26.1 -- not a known variable star
13:18:25.42 +73:11:59.8 -- not a known variable star
13:19:11.71 +73:25:37.5 -- a known variable star
13:19:32.20 +73:49:49.8 -- not a known variable star
13:19:34.04 +73:17:51.8 -- not a known variable star
13:19:46.85 +73:20:22.3 -- not a known variable star
13:20:11.43 +73:26:09.2 -- not a known variable star
13:21:06.13 +73:48:02.9 -- not a known variable star
13:22:31.96 +73:39:29.4 -- not a known variable star
13:22:47.96 +73:44:58.3 -- not a known variable star
13:23:25.77 +71:20:57.4 -- not a known variable star
13:23:39.26 +71:27:43.0 -- not a known variable star
13:25:07.32 +71:30:29.2 -- not a known variable star
13:25:45.11 +69:57:02.1 -- not a known variable star
13:26:41.19 +69:58:38.4 -- not a known variable star
13:26:50.03 +71:29:44.7 -- not a known variable star
13:27:03.14 +69:12:18.1 -- not a known variable star
13:33:45.63 +72:36:21.5 -- not a known variable star
Found 64 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
71 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 71 (excluding asteroids and hot pixels, 64 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)2461231.73293105 -observatory V36
07:32:34.83 +17:08:19.7 Mercury (5.1mag)
10:11:08.88 +12:44:05.9 Venus (-4.1mag)
04:23:49.25 +21:24:18.4 Mars (1.3mag)
08:16:34.10 +20:11:49.3 Jupiter (-1.8mag)
00:55:50.12 +03:20:26.0 Saturn (0.7mag)
04:07:12.66 +20:44:59.7 Uranus (5.8mag)
00:17:01.52 +00:20:41.8 Neptune (7.8mag)
20:30:55.60 -23:17:57.4 Pluto (14.4mag)
03:03:29.95 +21:39:35.9 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 361 Jul 10 00:54 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461231.73293105:
08:16:38.94 +20:11:33.3 Io (6.1mag)
08:16:34.87 +20:11:48.2 Europa (6.3mag)
08:16:50.69 +20:10:49.8 Ganymede (5.6mag)
08:17:02.52 +20:10:04.5 Callisto (6.8mag)
08:15:05.92 +19:55:55.9 Himalia (15.7mag)
08:16:32.19 +20:11:57.4 Thebe (16.6mag)
08:14:27.29 +20:00:27.1 Elara (17.6mag)
08:20:06.09 +20:06:03.1 Pasiphae (17.8mag)
08:21:32.35 +20:16:53.3 Carme (19.0mag)
00:55:39.71 +03:20:18.3 Titan (8.5mag)
00:55:44.96 +03:20:31.0 Rhea (9.8mag)
00:55:19.57 +03:19:36.3 Iapetus (11.2mag)
00:55:59.78 +03:20:44.2 Hyperion (14.5mag)
00:55:51.01 +03:17:40.8 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 00:54 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.73293105:
17:46:32.76 -33:02:20.5 JWST
15:58:36.20 +51:50:47.3 Chandra
20:21:03.35 +30:06:09.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 00:54 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.73293105 -observatory V36
02:36:05.97 +14:24:50.1 17.9mag P/1996 R2 (Lagerkvist)
18:18:02.05 -34:21:33.3 13.7mag P/2010 H2 (Vales)
06:25:33.28 -68:08:16.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:45.85 +32:26:41.8 17.6mag C/2017 K2 (PANSTARRS)
17:03:09.04 +16:02:56.7 18.0mag C/2021 G2 (ATLAS)
01:47:06.80 +07:58:47.2 15.4mag P/2021 N1 (ZTF)
22:59:36.13 +32:17:07.9 17.3mag C/2022 E2 (ATLAS)
06:12:15.75 +26:55:38.2 16.7mag C/2022 N2 (PANSTARRS)
09:55:24.68 +29:47:10.5 16.8mag C/2022 QE78 (ATLAS)
09:09:39.49 +04:59:48.7 17.8mag C/2022 R6 (PANSTARRS)
18:07:17.50 +21:17:53.9 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:36.01 -11:23:06.6 17.7mag P/2023 B1 (PANSTARRS)
21:49:22.69 +67:37:18.0 17.8mag C/2023 H5 (Lemmon)
16:31:07.42 -10:03:56.9 13.9mag C/2023 R1 (PANSTARRS)
08:00:26.59 +65:42:07.7 17.9mag C/2024 A1 (ATLAS)
07:32:39.39 +29:59:50.0 14.6mag C/2024 E1 (Wierzchos)
15:16:23.09 +15:19:30.5 17.5mag C/2024 G6 (ATLAS)
19:41:27.71 +39:22:09.9 13.8mag C/2024 J3 (ATLAS)
21:47:42.30 +45:59:06.2 17.8mag C/2024 R4 (PANSTARRS)
04:49:31.55 -13:48:04.9 15.7mag C/2024 T5 (ATLAS)
06:34:28.36 +29:05:22.7 18.0mag C/2025 J1 (Borisov)
07:14:15.14 -12:52:45.5 16.4mag C/2025 R3 (PANSTARRS)
09:55:57.21 +22:26:31.0 17.6mag C/2025 V2 (Rankin)
12:44:34.68 +03:56:34.1 17.1mag C/2025 Y1 (ATLAS)
16:52:18.10 +79:07:03.9 17.4mag C/2026 A2 (Bok)
02:46:08.78 +45:14:03.5 16.7mag C/2026 B2 (Sun-Gao)
11:25:26.13 +04:31:21.6 16.9mag A/2026 E1
21:18:51.56 -15:02:03.4 7.3mag 10P/Tempel
11:13:23.96 -01:52:55.9 16.1mag 29P/Schwassmann-Wachmann
03:59:59.92 +29:32:24.0 17.8mag 47P/Ashbrook-Jackson
10:07:49.53 +14:02:58.0 17.0mag 63P/Wild
00:48:18.56 -05:05:40.7 15.6mag 65P/Gunn
08:26:34.65 +34:13:27.8 17.9mag 76P/West-Kohoutek-Ikemura
04:27:06.45 +20:10:20.0 13.7mag 78P/Gehrels
02:22:08.29 +10:35:33.5 16.2mag 88P/Howell
06:35:10.28 +30:32:29.2 15.7mag 93P/Lovas
04:20:36.64 +31:07:02.6 16.9mag 114P/Wiseman-Skiff
08:08:24.03 +30:42:59.8 15.3mag 123P/West-Hartley
10:47:54.45 +01:14:08.0 16.8mag 124P/Mrkos
04:51:32.08 +20:48:33.7 16.2mag 128P/Shoemaker-Holt
05:36:01.68 +19:42:53.1 17.8mag 131P/Mueller
00:01:30.73 +02:55:49.5 17.9mag 139P/Vaisala-Oterma
07:13:06.88 +17:02:46.6 15.5mag 141P-D/Machholz
03:16:47.74 -21:06:57.1 15.5mag 161P/Hartley-IRAS
05:32:37.86 +33:55:19.8 15.3mag 162P/SidingSpring
19:04:46.88 +15:00:38.3 14.7mag 169P/NEAT
01:40:44.58 +07:35:05.1 17.7mag 220P/McNaught
16:35:59.39 -08:22:51.4 17.0mag 235P/LINEAR
08:45:01.88 +33:18:37.5 17.9mag 240P/NEAT
20:42:13.91 -49:32:36.4 17.8mag 259P/Garradd
01:58:58.31 +12:02:19.2 15.7mag 260P/McNaught
05:36:51.72 +36:49:58.4 17.4mag 295P/LINEAR
15:06:37.27 +06:04:02.8 17.6mag 391P/Kowalski
08:34:29.74 +19:40:53.8 17.9mag 450P/LONEOS
07:51:34.62 +39:13:33.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 00:54 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 00:54 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
20:52:11.463 -28:17:09.07 AT 2026spm 2026-07-07.32 21.7705
21:10:07.376 -16:54:40.86 AT 2026spl 2026-07-07.32 22.4035
-rw-r--r-- 1 apache apache 30K Jul 10 00:54 tns_transients_list.txt
